This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81
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 17.2466 2461208.7466 14.79 13:59:12.15 +26:18:45.4
33.70012 74.85744 galactic Boo Second-epoch detections are separated by 8.2" 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 | 13:59:12.15 +26:18:45.4 (user input) | T | P | (position from user input)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 13:59:12.15 +26:18:45.4: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 13:59:12.15 +26:18:45.4: 16.07 +/- 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,2461208.7466,14.79,0.05,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 20260617.2466 14.79CV 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 17.2466 2461208.7466 14.51 14:10:03.66 +26:06:47.2
34.09675 72.41643 galactic Boo Second-epoch detections are separated by 6.8" and 8.6 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 | 14:10:03.66 +26:06:47.2 (user input) | T | P | (position from user input)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:10:03.66 +26:06:47.2: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:10:03.66 +26:06:47.2: 16.01 +/- 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,2461208.7466,14.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260617.2466 14.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 06 17.2466 2461208.7466 14.75 13:58:29.15 +30:57:56.9
51.59801 74.86926 galactic CVn Second-epoch detections are separated by 6.1" 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 | 13:58:29.15 +30:57:56.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 13:58:29.15 +30:57:56.9: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 13:58:29.15 +30:57:56.9: 16.11 +/- 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,2461208.7466,14.75,0.05,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 20260617.2466 14.75CV 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 17.2466 2461208.7466 14.98 14:30:41.27 +27:16:40.9
39.05719 67.96806 galactic Boo Second-epoch detections are separated by 5.9" and 7.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 14:30:41.27 +27:16:40.9 (user input) | T | P | (position from user input)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:30:41.27 +27:16:40.9: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:30:41.27 +27:16:40.9: 15.79 +/- 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,2461208.7466,14.98,0.05,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 20260617.2466 14.98CV 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: 2461172.80993912 12.05.2026 07:26:08.740 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
First image: 2461172.80993912 12.05.2026 07:26:08.740 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
Last image: 2461208.74690556 17.06.2026 05:55:22.640 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 21
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.43
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 4636
Objects passed selection criteria: 4634
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 4436.5
Average stars matched: 4250.25 (95.8019 %)
Memory usage VmPeak: 111060 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 Wed Jun 17 01:13:14 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: 2461172.80993912 12.05.2026 07:26:08.740 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
First image: 2461172.80993912 12.05.2026 07:26:08.740 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
Last image: 2461208.74690556 17.06.2026 05:55:22.640 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 149
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.12
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: 22 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): 25011
Objects passed selection criteria: 24955
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 29279
Average stars matched: 23470.5 (80.1615 %)
Memory usage VmPeak: 135180 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 Wed Jun 17 01:15:06 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:
CVn-03-Q2b1x1
#######################################
########### Starting CVn-03-Q2b1x1 ###########
Processing CVn-03-Q2b1x1
WARNING: server tau is low on disk space, only 69299 MB free at /data_ssd/NMW-TexasTech/workdir
WARNING: server tau is low on disk space, only 69299 MB free at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.png' -> 'transient_report/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits_preview.png'
CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
renamed 'CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.png' -> 'transient_report/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits_preview.png'
CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.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= 441.6545
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 449.7903
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 928.9168
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 455.1004
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 929.4571
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 455.0203
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.10327
INFO: SECOND_EPOCH__SD_ratio= 0.000
----------------------------------------------
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 = 26.2299995422363 / [degC] Focuser temperature
AMBTEMP = 26.6 / [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_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
EXPTIME = 20.0 / [s] Exposure duration
SET-TEMP= 10.0 / [degC] CCD temperature setpoint
CCD-TEMP= 10.0 / [degC] CCD temperature
FOCTEMP = 25.4799995422363 / [degC] Focuser temperature
AMBTEMP = 26.6 / [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_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.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/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
SExtractor catalog cache: saved CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.cat to cache
SExtractor catalog cache: saved CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.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/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.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: 2461208.74637028
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_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits exists and is non-empty
Saving wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits to local_wcs_cache/
'wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits' -> 'local_wcs_cache/wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits'
wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits exists and is non-empty
Saving wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits to local_wcs_cache/
'wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits' -> 'local_wcs_cache/wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits'
wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits exists and is non-empty
Saving wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits to local_wcs_cache/
'wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits' -> 'local_wcs_cache/wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits'
wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits exists and is non-empty
Saving wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits to local_wcs_cache/
'wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits' -> 'local_wcs_cache/wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits (1st reference image)
verification OK: wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:59:54.041 +29:59:36.81 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits (1st new image)
verification OK: wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
Image size: 936.9'x623.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:00:00.474 +30:00:07.84 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:59:54.041 +29:59:36.81
Second-epoch image center 14:00:00.474 +30:00:07.84
Angular distance between the image centers 0.0248 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits (2nd new image)
verification OK: wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
Image size: 936.9'x623.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:00:02.698 +30:00:41.91 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:59:54.041 +29:59:36.81
Second-epoch image center 14:00:02.698 +30:00:41.91
Angular distance between the image centers 0.0361 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 14:00:00.474 +30:00:07.84
Second-epoch second image center 14:00:02.698 +30:00:41.91
Angular distance between the image centers 0.01241 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/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits &> /tmp/tmp.WKb7le4jZY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits &> /tmp/tmp.CxMwtdeGmr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits &> /tmp/tmp.LmYVQPTX51
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits &> /tmp/tmp.upcRUxShID
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
Calibrating the magnitude scale
Found non-empty wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.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_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits and wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.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_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits and wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat
Found non-empty wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits and wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat
The reference image (wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits) and catalog (wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat) found
'wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat' -> 'wcsmag.cat'
Read 5741 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 200.7878 to 219.7278 deg, Dec +24.1050 to +35.4406 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 200.7878 to 219.7278 deg, Dec 24.1050 to 35.4406 deg
Loaded 4627 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): 3339 out of 3475 total matches.
Matched with Tycho-2 3475 out of 5741 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.826300
a=0.000000 b=1.000000 c=22.826300
From vast_summary.log: estimated ref. image limiting mag.: -7.43
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.40
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.40
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 5741 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 200.7878 to 219.7278 deg, Dec +24.1050 to +35.4406 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 200.7878 to 219.7278 deg, Dec 24.1050 to 35.4406 deg
Loaded 4627 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): 3339 out of 3475 total matches.
Matched with Tycho-2 3475 out of 5741 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits:
Forced-photometry filter: calibrated wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits -> calib.txt_param_ref_wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits (aperture=6.3)
Read 5486 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 200.5276 to 219.4457 deg, Dec +24.5781 to +35.2411 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 200.5276 to 219.4457 deg, Dec 24.5781 to 35.2411 deg
Loaded 4374 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): 3394 out of 3470 total matches.
Matched with Tycho-2 3470 out of 5486 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits:
Forced-photometry filter: calibrated wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits -> calib.txt_param_ref_wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 21 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
2.3 pix CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
2.3 pix CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
2.3 pix CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
2.2 pix wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
2.3 pix wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
Limiting magnitude estimates:
15.4 mag. CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
15.2 mag. CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
15.3 mag. CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
15.3 mag. CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.3 (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.WKb7le4jZY (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/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.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_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits' -> 'wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
WCS_IMAGE_NAME=wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
WCS-calibrated image found: wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
Checking if the catalog wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat corresponding to the image wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits alredy exist and is non-empty...
Catalog wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat corresponding to the image wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
WCS catalog name: wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=365, passed=5741
Got 5741 stars (including 5372 good ones) from the SExtractor catalog wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat
util/solve_plate_with_UCAC5 got 5741 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 963 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 963 matched stars entering correct_measured_positions(), 5682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 5682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 5682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 964 stars left (next iteration limit 1059)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits N_match=964 sigma_overall_arcsec=0.342 sigma_q1_arcsec=0.343 sigma_q2_arcsec=0.445 sigma_q3_arcsec=0.291 sigma_q4_arcsec=0.331 n_q1=264 n_q2=234 n_q3=247 n_q4=219 worst_quadrant_to_overall_ratio=1.303
The image catalog is written to wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits -region wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.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.CxMwtdeGmr (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_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits' -> 'wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
WCS_IMAGE_NAME=wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
WCS-calibrated image found: wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
Checking if the catalog wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits.wcscat corresponding to the image wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits alredy exist and is non-empty...
Catalog wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits.wcscat corresponding to the image wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
WCS catalog name: wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=263, passed=5486
Got 5486 stars (including 5221 good ones) from the SExtractor catalog wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits.wcscat
util/solve_plate_with_UCAC5 got 5486 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.6 to 35.2)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 5396 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 572 to 628 (Dec 24.6 to 35.2)
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 5396 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 967 matched stars entering correct_measured_positions(), 5396 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits N_match=967 sigma_overall_arcsec=0.410 sigma_q1_arcsec=0.294 sigma_q2_arcsec=0.449 sigma_q3_arcsec=0.425 sigma_q4_arcsec=0.464 n_q1=259 n_q2=264 n_q3=215 n_q4=229 worst_quadrant_to_overall_ratio=1.132
The image catalog is written to wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits -region wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.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.LmYVQPTX51 (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_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.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_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
WCS_IMAGE_NAME=wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
WCS-calibrated image found: wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
Checking if the catalog wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits.wcscat corresponding to the image wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits alredy exist and is non-empty...
Catalog wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits.wcscat corresponding to the image wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
WCS catalog name: wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=331, passed=5476
Got 5476 stars (including 5145 good ones) from the SExtractor catalog wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits.wcscat
util/solve_plate_with_UCAC5 got 5476 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 573 to 628 (Dec 24.6 to 35.2)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 944 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 5353 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 573 to 628 (Dec 24.6 to 35.2)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 5354 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 5360 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 965 stars left (next iteration limit 1061)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits N_match=965 sigma_overall_arcsec=0.382 sigma_q1_arcsec=0.283 sigma_q2_arcsec=0.481 sigma_q3_arcsec=0.381 sigma_q4_arcsec=0.409 n_q1=254 n_q2=269 n_q3=215 n_q4=227 worst_quadrant_to_overall_ratio=1.260
The image catalog is written to wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits -region wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.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.upcRUxShID (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_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.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_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
WCS_IMAGE_NAME=wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
WCS-calibrated image found: wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
Checking if the catalog wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits.wcscat corresponding to the image wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits alredy exist and is non-empty...
Catalog wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits.wcscat corresponding to the image wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
WCS catalog name: wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=343, passed=5524
Got 5524 stars (including 5180 good ones) from the SExtractor catalog wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits.wcscat
util/solve_plate_with_UCAC5 got 5524 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 573 to 628 (Dec 24.6 to 35.3)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 945 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 5374 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 573 to 628 (Dec 24.6 to 35.3)
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 5375 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 965 matched stars entering correct_measured_positions(), 5380 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 965 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits N_match=965 sigma_overall_arcsec=0.354 sigma_q1_arcsec=0.273 sigma_q2_arcsec=0.437 sigma_q3_arcsec=0.353 sigma_q4_arcsec=0.407 n_q1=255 n_q2=272 n_q3=213 n_q4=225 worst_quadrant_to_overall_ratio=1.232
The image catalog is written to wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits -region wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.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=CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits sigma_overall=0.342 worst_q_ratio=1.303
ref2=CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits sigma_overall=0.410 worst_q_ratio=1.132
new1=CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits sigma_overall=0.382 worst_q_ratio=1.260
new2=CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits sigma_overall=0.354 worst_q_ratio=1.232
reference average sigma_overall=0.376 worst_q_ratio=1.2175
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257_astrometric_residuals.png (964 matched stars from wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.31 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603_astrometric_residuals.png (967 matched stars from wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204_astrometric_residuals.png (965 matched stars from wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.33 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205_astrometric_residuals.png (965 matched stars from wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.32 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits'
Saving fully-calibrated image wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits'
Preparing the HTML report for the field CVn-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:08:20.78 +29:34:14.3: 12.57 +/- 0.01 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 13:49:48.53 +28:38:08.3: 12.51 +/- 0.01 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:00:31.68 +29:29:04.8: 12.46 +/- 0.01 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:05:24.90 +29:24:21.5: 12.57 +/- 0.01 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:02:04.82 +30:07:32.7: 12.43 +/- 0.01 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 13:54:58.43 +31:53:53.2: 12.57 +/- 0.01 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:03:57.25 +29:49:06.9: 12.61 +/- 0.01 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 13:59:07.91 +30:49:32.0: 12.62 +/- 0.01 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 13:53:04.98 +29:20:53.7: 12.59 +/- 0.01 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:02:37.98 +31:17:12.5: 12.63 +/- 0.01 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 13:49:48.53 +28:38:08.3: 12.47 +/- 0.01 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:08:20.78 +29:34:14.3: 12.54 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry reference-image weighted average: 12.49 +/- 0.01
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 13:54:58.43 +31:53:53.2: 12.55 +/- 0.01 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:00:31.68 +29:29:04.8: 12.41 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 13:49:48.53 +28:38:08.3: ref_mag=12.49 +/- 0.01 new_mean_mag=12.3589 delta=0.13 (need > 0.90)
Forced photometry filter REJECTED candidate at 14:08:20.78 +29:34:14.3: ref_mag=12.56 +/- 0.01 new_mean_mag=12.3428 delta=0.21 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:05:24.90 +29:24:21.5: 12.51 +/- 0.02 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:03:57.25 +29:49:06.9: 12.55 +/- 0.02 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:02:04.82 +30:07:32.7: 12.40 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.44 +/- 0.01
Forced photometry reference-image weighted average: 12.56 +/- 0.01
Forced photometry reference-image weighted average: 12.54 +/- 0.01
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry filter REJECTED candidate at 14:00:31.68 +29:29:04.8: ref_mag=12.44 +/- 0.01 new_mean_mag=12.1929 delta=0.25 (need > 0.90)
Forced photometry filter REJECTED candidate at 13:54:58.43 +31:53:53.2: ref_mag=12.56 +/- 0.01 new_mean_mag=12.3636 delta=0.20 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 13:59:07.91 +30:49:32.0: 12.53 +/- 0.01 detection
Forced photometry filter REJECTED candidate at 14:05:24.90 +29:24:21.5: ref_mag=12.54 +/- 0.01 new_mean_mag=12.3313 delta=0.21 (need > 0.90)
Forced photometry reference-image weighted average: 12.42 +/- 0.01
Forced photometry filter REJECTED candidate at 14:03:57.25 +29:49:06.9: ref_mag=12.58 +/- 0.01 new_mean_mag=12.3555 delta=0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 14:02:04.82 +30:07:32.7: ref_mag=12.42 +/- 0.01 new_mean_mag=12.2334 delta=0.19 (need > 0.90)
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter REJECTED candidate at 13:59:07.91 +30:49:32.0: ref_mag=12.57 +/- 0.01 new_mean_mag=12.3491 delta=0.23 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 13:53:04.98 +29:20:53.7: 12.55 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:02:37.98 +31:17:12.5: 12.56 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 13:53:04.98 +29:20:53.7: ref_mag=12.57 +/- 0.01 new_mean_mag=12.3778 delta=0.19 (need > 0.90)
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry filter REJECTED candidate at 14:02:37.98 +31:17:12.5: ref_mag=12.60 +/- 0.01 new_mean_mag=12.3982 delta=0.20 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:04:46.27 +31:37:21.9: 12.58 +/- 0.01 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 13:56:16.27 +30:22:58.8: 12.67 +/- 0.02 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:05:06.97 +30:15:08.4: 12.66 +/- 0.02 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:08:44.32 +29:54:13.1: 12.64 +/- 0.02 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:03:36.16 +27:37:36.5: 12.61 +/- 0.02 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 13:53:48.19 +31:42:43.7: 12.66 +/- 0.02 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:04:46.27 +31:37:21.9: 12.61 +/- 0.02 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:05:06.97 +30:15:08.4: 12.63 +/- 0.02 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 13:56:16.27 +30:22:58.8: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter REJECTED candidate at 14:04:46.27 +31:37:21.9: ref_mag=12.59 +/- 0.01 new_mean_mag=12.4387 delta=0.15 (need > 0.90)
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry reference-image weighted average: 12.66 +/- 0.01
Forced photometry filter REJECTED candidate at 14:05:06.97 +30:15:08.4: ref_mag=12.65 +/- 0.01 new_mean_mag=12.3929 delta=0.25 (need > 0.90)
Forced photometry filter REJECTED candidate at 13:56:16.27 +30:22:58.8: ref_mag=12.66 +/- 0.01 new_mean_mag=12.4547 delta=0.21 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 13:53:48.19 +31:42:43.7: 12.64 +/- 0.02 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:03:36.16 +27:37:36.5: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:08:44.32 +29:54:13.1: 12.60 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry filter REJECTED candidate at 13:53:48.19 +31:42:43.7: ref_mag=12.65 +/- 0.01 new_mean_mag=12.4500 delta=0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 14:03:36.16 +27:37:36.5: ref_mag=12.60 +/- 0.01 new_mean_mag=12.4257 delta=0.18 (need > 0.90)
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter REJECTED candidate at 14:08:44.32 +29:54:13.1: ref_mag=12.63 +/- 0.01 new_mean_mag=12.4202 delta=0.21 (need > 0.90)
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
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Considering the candidate 20312_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20312_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 20313_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20313_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 20316_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20316_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 20317_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20317_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
**** FOUND 13:58:34.49 +30:56:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20318_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20318_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 20319_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20319_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 20320_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20320_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
**** FOUND 13:56:48.90 +28:44:19.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20321_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20321_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 20322_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20322_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 20323_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20323_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 20324_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20324_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 20326_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20326_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 20327_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20327_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 20328_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20328_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 20329_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20329_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
**** FOUND 14:02:43.88 +30:36:16.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20330_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20330_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 20331_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20331_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 20332_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20332_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 20333_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20333_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 20334_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20334_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
**** FOUND 13:58:05.54 +27:36:00.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20335_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 20335_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
**** FOUND 13:57:33.64 +31:24:35.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field CVn-03-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/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
SExtractor catalog cache: saved CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.cat to cache
SExtractor catalog cache: saved CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
Creating symlink local_wcs_cache/wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
Creating symlink local_wcs_cache/wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
Creating symlink local_wcs_cache/wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.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_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits exists and is non-empty
wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits exists and is non-empty
wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits exists and is non-empty
wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits (1st reference image)
verification OK: wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
Image size: 941.3'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 13:59:54.041 +29:59:36.81 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits (1st new image)
verification OK: wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
Image size: 936.9'x623.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:00:00.474 +30:00:07.84 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 13:59:54.041 +29:59:36.81
Second-epoch image center 14:00:00.474 +30:00:07.84
Angular distance between the image centers 0.0248 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits (2nd new image)
verification OK: wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
Image size: 936.9'x623.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 14:00:02.698 +30:00:41.91 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 13:59:54.041 +29:59:36.81
Second-epoch image center 14:00:02.698 +30:00:41.91
Angular distance between the image centers 0.0361 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 14:00:00.474 +30:00:07.84
Second-epoch second image center 14:00:02.698 +30:00:41.91
Angular distance between the image centers 0.01241 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/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits &> /tmp/tmp.QwUYhNoYn2
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits &> /tmp/tmp.9568CamtUV
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits &> /tmp/tmp.3aiGQ1sTEH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits &> /tmp/tmp.dBI35nAchF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
Calibrating the magnitude scale
Found non-empty wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.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_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits and wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.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_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits and wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat
Found non-empty wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits and wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat
The reference image (wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits) and catalog (wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat) found
'wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat' -> 'wcsmag.cat'
Read 32125 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 200.7878 to 219.7982 deg, Dec +24.0584 to +35.4473 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 200.7878 to 219.7982 deg, Dec 24.0584 to 35.4473 deg
Loaded 4683 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): 3242 out of 3520 total matches.
Matched with Tycho-2 3520 out of 32125 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.704050
a=0.000000 b=1.000000 c=22.704050
From vast_summary.log: estimated ref. image limiting mag.: -7.12
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.58
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.58
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 32125 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 200.7878 to 219.7982 deg, Dec +24.0584 to +35.4473 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 200.7878 to 219.7982 deg, Dec 24.0584 to 35.4473 deg
Loaded 4683 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): 3242 out of 3520 total matches.
Matched with Tycho-2 3520 out of 32125 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits:
Forced-photometry filter: calibrated wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits -> calib.txt_param_ref_wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits (aperture=4.8)
Read 28454 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 200.4711 to 219.4750 deg, Dec +24.5099 to +35.2604 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 200.4711 to 219.4750 deg, Dec 24.5099 to 35.2604 deg
Loaded 4426 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): 3312 out of 3504 total matches.
Matched with Tycho-2 3504 out of 28454 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits:
Forced-photometry filter: calibrated wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits -> calib.txt_param_ref_wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 44 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
2.2 pix CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
2.4 pix CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
2.4 pix CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
2.0 pix wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
2.2 pix wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
Limiting magnitude estimates:
15.6 mag. CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
15.4 mag. CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
15.5 mag. CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
15.5 mag. CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 14.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.QwUYhNoYn2 (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/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.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_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits 574.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits' -> 'wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
WCS_IMAGE_NAME=wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
WCS-calibrated image found: wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
Checking if the catalog wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat corresponding to the image wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits alredy exist and is non-empty...
Catalog wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat corresponding to the image wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits
WCS catalog name: wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=29, blended=1187, passed=32096
Got 32096 stars (including 30851 good ones) from the SExtractor catalog wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat
util/solve_plate_with_UCAC5 got 32096 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 952 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 31681 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 570 to 629 (Dec 24.1 to 35.4)
Done reading UCAC5 zone files...
Matched 964 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 31682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 964 matched stars entering correct_measured_positions(), 31682 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits N_match=964 sigma_overall_arcsec=0.327 sigma_q1_arcsec=0.320 sigma_q2_arcsec=0.405 sigma_q3_arcsec=0.277 sigma_q4_arcsec=0.326 n_q1=265 n_q2=242 n_q3=247 n_q4=210 worst_quadrant_to_overall_ratio=1.241
The image catalog is written to wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits -region wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.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.9568CamtUV (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_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits' -> 'wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
WCS_IMAGE_NAME=wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
WCS-calibrated image found: wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
Checking if the catalog wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits.wcscat corresponding to the image wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits alredy exist and is non-empty...
Catalog wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits.wcscat corresponding to the image wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits
WCS catalog name: wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1014, passed=28443
Got 28443 stars (including 27395 good ones) from the SExtractor catalog wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits.wcscat
util/solve_plate_with_UCAC5 got 28443 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 28022 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
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 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 28022 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 968 matched stars entering correct_measured_positions(), 28022 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits N_match=968 sigma_overall_arcsec=0.419 sigma_q1_arcsec=0.278 sigma_q2_arcsec=0.478 sigma_q3_arcsec=0.434 sigma_q4_arcsec=0.477 n_q1=260 n_q2=265 n_q3=215 n_q4=228 worst_quadrant_to_overall_ratio=1.141
The image catalog is written to wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits -region wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.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.3aiGQ1sTEH (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_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.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_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
WCS_IMAGE_NAME=wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
WCS-calibrated image found: wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
Checking if the catalog wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits.wcscat corresponding to the image wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits alredy exist and is non-empty...
Catalog wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits.wcscat corresponding to the image wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
WCS catalog name: wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=8, blended=1692, passed=41011
Got 41011 stars (including 39227 good ones) from the SExtractor catalog wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits.wcscat
util/solve_plate_with_UCAC5 got 41011 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 902 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 39037 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 932 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 39038 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 931 matched stars entering correct_measured_positions(), 39037 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 931 stars left (next iteration limit 1024)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits N_match=931 sigma_overall_arcsec=0.354 sigma_q1_arcsec=0.280 sigma_q2_arcsec=0.436 sigma_q3_arcsec=0.355 sigma_q4_arcsec=0.366 n_q1=270 n_q2=241 n_q3=220 n_q4=200 worst_quadrant_to_overall_ratio=1.230
The image catalog is written to wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits -region wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.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.dBI35nAchF (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_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.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_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
WCS_IMAGE_NAME=wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
WCS-calibrated image found: wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
Checking if the catalog wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits.wcscat corresponding to the image wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits alredy exist and is non-empty...
Catalog wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits.wcscat corresponding to the image wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
WCS catalog name: wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1705, passed=40642
Got 40642 stars (including 38847 good ones) from the SExtractor catalog wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits.wcscat
util/solve_plate_with_UCAC5 got 40642 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 936.9'
Seting catalog search parameters based on the expected field of view 936.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013013 (46.8 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010410 (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 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 38618 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
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 572 to 628 (Dec 24.5 to 35.3)
Done reading UCAC5 zone files...
Matched 928 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 38618 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 38618 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 928 stars left (next iteration limit 1020)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits N_match=928 sigma_overall_arcsec=0.337 sigma_q1_arcsec=0.268 sigma_q2_arcsec=0.418 sigma_q3_arcsec=0.336 sigma_q4_arcsec=0.362 n_q1=266 n_q2=245 n_q3=214 n_q4=203 worst_quadrant_to_overall_ratio=1.241
The image catalog is written to wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits -region wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.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_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.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_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/wcs_CVn-03-Q2b1x1_2026-06-17_00-54-36_20.00sec_10.00C_LIGHT_0204.fits
Saving fully-calibrated image wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.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_2026-06-17_CI_CVn-03-Q2b1x1_011103_TTUQ2b1x1_3773171_PzXzhP81/wcs_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205.fits
Preparing the HTML report for the field CVn-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:24:40.93 +28:10:37.9: 15.37 +/- 0.19 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:05:33.41 +28:32:15.4: 14.68 +/- 0.18 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:30:56.29 +31:28:15.9: 14.57 +/- 0.10 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:11:23.26 +33:03:21.3: 14.59 +/- 0.09 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:29:25.07 +26:47:22.5: 14.55 +/- 0.10 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:30:10.38 +27:57:46.7: 14.26 +/- 0.08 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 13:42:26.75 +33:15:28.8: 14.05 +/- 0.05 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:21:06.29 +27:17:37.2: 14.24 +/- 0.07 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 13:40:42.15 +30:54:04.3: 14.73 +/- 0.10 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 13:40:16.44 +29:45:58.3: 14.23 +/- 0.06 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:24:40.93 +28:10:37.9: 15.03 +/- 0.15 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:05:33.41 +28:32:15.4: 14.73 +/- 0.18 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 13:42:26.75 +33:15:28.8: 14.05 +/- 0.06 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:29:25.07 +26:47:22.5: 14.90 +/- 0.16 detection
Forced photometry reference-image weighted average: 15.16 +/- 0.12
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:11:23.26 +33:03:21.3: 14.57 +/- 0.10 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:30:56.29 +31:28:15.9: 14.86 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.05 +/- 0.04
Forced photometry reference-image weighted average: 14.70 +/- 0.13
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:30:10.38 +27:57:46.7: 14.24 +/- 0.08 detection
Forced photometry filter REJECTED candidate at 14:24:40.93 +28:10:37.9: ref_mag=15.16 +/- 0.12 new_mean_mag=14.9294 delta=0.23 (need > 0.90)
Forced photometry filter REJECTED candidate at 13:42:26.75 +33:15:28.8: ref_mag=14.05 +/- 0.04 new_mean_mag=14.3547 delta=-0.30 (need > 0.90)
Forced photometry filter REJECTED candidate at 14:05:33.41 +28:32:15.4: ref_mag=14.70 +/- 0.13 new_mean_mag=14.4930 delta=0.21 (need > 0.90)
Forced photometry reference-image weighted average: 14.65 +/- 0.09
Forced photometry reference-image weighted average: 14.66 +/- 0.08
Forced photometry reference-image weighted average: 14.58 +/- 0.06
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 13:40:42.15 +30:54:04.3: 14.69 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.25 +/- 0.06
Forced photometry filter REJECTED candidate at 14:29:25.07 +26:47:22.5: ref_mag=14.65 +/- 0.09 new_mean_mag=14.9540 delta=-0.31 (need > 0.90)
Forced photometry filter REJECTED candidate at 14:30:56.29 +31:28:15.9: ref_mag=14.66 +/- 0.08 new_mean_mag=14.7769 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 14:11:23.26 +33:03:21.3: ref_mag=14.58 +/- 0.06 new_mean_mag=14.3730 delta=0.21 (need > 0.90)
Forced photometry filter REJECTED candidate at 14:30:10.38 +27:57:46.7: ref_mag=14.25 +/- 0.06 new_mean_mag=14.4034 delta=-0.16 (need > 0.90)
Forced photometry reference-image weighted average: 14.71 +/- 0.07
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:21:06.29 +27:17:37.2: 14.28 +/- 0.08 detection
Forced photometry filter REJECTED candidate at 13:40:42.15 +30:54:04.3: ref_mag=14.71 +/- 0.07 new_mean_mag=14.9544 delta=-0.24 (need > 0.90)
Forced photometry reference-image weighted average: 14.26 +/- 0.05
Forced photometry filter REJECTED candidate at 14:21:06.29 +27:17:37.2: ref_mag=14.26 +/- 0.05 new_mean_mag=14.2202 delta=0.04 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 13:40:16.44 +29:45:58.3: 14.26 +/- 0.07 detection
Forced photometry reference-image weighted average: 14.24 +/- 0.04
Forced photometry filter REJECTED candidate at 13:40:16.44 +29:45:58.3: ref_mag=14.24 +/- 0.04 new_mean_mag=14.6277 delta=-0.39 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:06:41.78 +26:29:59.3: 14.38 +/- 0.07 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:05:42.98 +28:44:47.5: 13.09 +/- 0.02 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:11:19.87 +28:05:59.4: 12.21 +/- 0.01 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:01:30.83 +31:34:07.3: 14.43 +/- 0.08 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 13:59:12.15 +26:18:45.4: 16.14 +/- 99.00 upperlimit
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:00:15.32 +30:57:37.1: 14.61 +/- 0.08 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:10:03.66 +26:06:47.2: 16.16 +/- 99.00 upperlimit
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 13:52:11.42 +30:47:55.8: 15.63 +/- 0.21 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 13:58:29.15 +30:57:56.9: 16.27 +/- 99.00 upperlimit
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 13:56:37.67 +28:21:44.5: 15.13 +/- 0.14 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:06:41.78 +26:29:59.3: 14.32 +/- 0.08 detection
Forced photometry reference-image weighted average: 14.35 +/- 0.05
Forced photometry filter REJECTED candidate at 14:06:41.78 +26:29:59.3: ref_mag=14.35 +/- 0.05 new_mean_mag=14.1657 delta=0.19 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:05:42.98 +28:44:47.5: 13.04 +/- 0.02 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:11:19.87 +28:05:59.4: 12.17 +/- 0.01 detection
Forced photometry reference-image weighted average: 13.07 +/- 0.01
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:01:30.83 +31:34:07.3: 14.68 +/- 0.12 detection
Forced photometry reference-image weighted average: 12.19 +/- 0.01
Forced photometry filter REJECTED candidate at 14:05:42.98 +28:44:47.5: ref_mag=13.07 +/- 0.01 new_mean_mag=13.0065 delta=0.06 (need > 0.90)
Forced photometry filter REJECTED candidate at 14:11:19.87 +28:05:59.4: ref_mag=12.19 +/- 0.01 new_mean_mag=12.0155 delta=0.17 (need > 0.90)
Forced photometry reference-image weighted average: 14.51 +/- 0.07
Forced photometry filter REJECTED candidate at 14:01:30.83 +31:34:07.3: ref_mag=14.51 +/- 0.07 new_mean_mag=14.4265 delta=0.08 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 13:59:12.15 +26:18:45.4: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:00:15.32 +30:57:37.1: 14.95 +/- 0.12 detection
Forced photometry reference-image weighted average: 14.71 +/- 0.07
Forced photometry filter REJECTED candidate at 14:00:15.32 +30:57:37.1: ref_mag=14.71 +/- 0.07 new_mean_mag=14.6161 delta=0.09 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:10:03.66 +26:06:47.2: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 13:52:11.42 +30:47:55.8: 15.57 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.60 +/- 0.15
Forced photometry filter REJECTED candidate at 13:52:11.42 +30:47:55.8: ref_mag=15.60 +/- 0.15 new_mean_mag=14.7725 delta=0.83 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 13:56:37.67 +28:21:44.5: 14.96 +/- 0.14 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 13:58:29.15 +30:57:56.9: 16.11 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 15.04 +/- 0.10
Forced photometry filter REJECTED candidate at 13:56:37.67 +28:21:44.5: ref_mag=15.04 +/- 0.10 new_mean_mag=14.8553 delta=0.19 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:07:40.49 +29:40:37.2: 15.55 +/- 0.20 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:20:49.61 +25:58:43.1: 15.07 +/- 0.15 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:12:58.40 +27:14:12.6: 14.99 +/- 0.12 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:29:24.26 +32:08:01.8: 14.71 +/- 0.11 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:21:10.03 +30:40:50.1: 15.58 +/- 0.20 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:21:02.31 +30:51:55.3: 15.06 +/- 0.13 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:07:40.49 +29:40:37.2: 15.49 +/- 0.21 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:20:49.61 +25:58:43.1: 15.23 +/- 0.20 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:18:23.00 +28:57:01.7: 15.57 +/- 0.22 detection
Forced photometry reference-image weighted average: 15.52 +/- 0.14
Forced photometry filter REJECTED candidate at 14:07:40.49 +29:40:37.2: ref_mag=15.52 +/- 0.14 new_mean_mag=14.9199 delta=0.60 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:29:24.26 +32:08:01.8: 15.35 +/- 0.23 detection
Forced photometry reference-image weighted average: 15.12 +/- 0.12
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:12:58.40 +27:14:12.6: 15.52 +/- 0.23 detection
Forced photometry filter REJECTED candidate at 14:20:49.61 +25:58:43.1: ref_mag=15.12 +/- 0.12 new_mean_mag=14.8753 delta=0.25 (need > 0.90)
Forced photometry reference-image weighted average: 14.82 +/- 0.10
Forced photometry reference-image weighted average: 15.11 +/- 0.11
Forced photometry filter REJECTED candidate at 14:29:24.26 +32:08:01.8: ref_mag=14.82 +/- 0.10 new_mean_mag=14.9023 delta=-0.08 (need > 0.90)
Forced photometry filter REJECTED candidate at 14:12:58.40 +27:14:12.6: ref_mag=15.11 +/- 0.11 new_mean_mag=14.9667 delta=0.15 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:21:10.03 +30:40:50.1: 15.82 +/- 0.31 detection
Forced photometry reference-image weighted average: 15.65 +/- 0.17
Forced photometry filter REJECTED candidate at 14:21:10.03 +30:40:50.1: ref_mag=15.65 +/- 0.17 new_mean_mag=14.9765 delta=0.68 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:21:02.31 +30:51:55.3: 15.27 +/- 0.19 detection
Forced photometry reference-image weighted average: 15.13 +/- 0.11
Forced photometry filter REJECTED candidate at 14:21:02.31 +30:51:55.3: ref_mag=15.13 +/- 0.11 new_mean_mag=14.9496 delta=0.18 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:18:23.00 +28:57:01.7: 15.19 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.33 +/- 0.14
Forced photometry filter REJECTED candidate at 14:18:23.00 +28:57:01.7: ref_mag=15.33 +/- 0.14 new_mean_mag=14.9224 delta=0.41 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:30:31.54 +30:33:36.7: 15.58 +/- 0.24 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:20:55.59 +31:32:51.6: 14.93 +/- 0.12 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-12_02-26-08_20.00sec_-4.90C_LIGHTs_0257.fits at 14:30:41.27 +27:16:40.9: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:20:55.59 +31:32:51.6: 15.06 +/- 0.16 detection
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:30:31.54 +30:33:36.7: 14.86 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.97 +/- 0.09
Forced photometry filter REJECTED candidate at 14:20:55.59 +31:32:51.6: ref_mag=14.97 +/- 0.09 new_mean_mag=14.8680 delta=0.10 (need > 0.90)
Forced photometry reference-image weighted average: 15.05 +/- 0.12
Forced photometry filter REJECTED candidate at 14:30:31.54 +30:33:36.7: ref_mag=15.05 +/- 0.12 new_mean_mag=14.9674 delta=0.09 (need > 0.90)
Forced photometry on wcs_CVn-03-Q2b1x1_2026-05-18_01-23-40_20.00sec_5.00C_LIGHT_1603.fits at 14:30:41.27 +27:16:40.9: 15.79 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out54720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55379.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out55743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out60043.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 20s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 51565_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 51565_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 51566_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 51566_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 51572_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 51572_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 51595_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 51595_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 51600_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 51600_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 51604_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 51604_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 51613_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 51613_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 51614_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 51614_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 51616_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 51616_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 51620_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 51620_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 51622_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 51622_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
**** FOUND 14:05:26.33 +28:30:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 51624_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 51624_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 51631_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 51631_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 51634_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 51634_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 52918_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 52918_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 53235_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 53235_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
**** FOUND 14:11:29.95 +28:03:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 54518_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 54518_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
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Considering the candidate 54717_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 54717_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 54720_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
Preparing report for the candidate 54720_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
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Considering the candidate 54742_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 54742_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 55379_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
Preparing report for the candidate 55379_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
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Considering the candidate 55646_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 55646_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 55714_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 55714_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 55743_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
Preparing report for the candidate 55743_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
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Considering the candidate 56286_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 56286_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 56521_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 56521_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
Rejecting candidate due to large distance (21.2") between the two second-epoch detections
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Considering the candidate 56944_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 56944_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
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Considering the candidate 56980_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 56980_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 57003_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 57003_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 57236_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 57236_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 57289_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 57289_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 57440_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 57440_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 57476_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 57476_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 57508_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 57508_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
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Considering the candidate 58598_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 58598_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 58840_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 58840_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 58963_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 58963_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 59016_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 59016_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 59021_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 59021_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 59337_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 59337_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 59362_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 59362_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
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Considering the candidate 59368_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 59368_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 60006_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205
The candidate 60006_CVn-03-Q2b1x1_2026-06-17_00-55-22_20.00sec_10.00C_LIGHT_0205 did not pass the final checks
