This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku
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 17.2502 2461208.7502 12.50 15:42:52.76 +06:03:38.6
13.51648 44.17650 galactic Ser Second-epoch detections are separated by 0.2" and 10.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.660 Crescentia -0 -0 0 12.6 0 -0
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:42:52.76 +06:03:38.6: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:42:52.76 +06:03:38.6: 15.78 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 17.2502* 15 42 52.76 +06 03 38.6 12.5 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461208.7502,12.50,0.05,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
VARIABLE_NAME 20260617.2502 12.50CV 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 17.2502 2461208.7502 12.81 15:19:19.61 +01:52:17.4
3.79799 46.51444 galactic Ser Second-epoch detections are separated by 0.5" and 10.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.173 Ino -0 -0 0 12.9 -0 0
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:19:19.61 +01:52:17.4: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:19:19.61 +01:52:17.4: 15.95 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 17.2502* 15 19 19.61 +01 52 17.4 12.8 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461208.7502,12.81,0.05,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
VARIABLE_NAME 20260617.2502 12.81CV 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 17.2502 2461208.7502 13.33 15:29:29.00 +07:36:00.4
12.81510 47.80817 galactic Ser Second-epoch detections are separated by 0.4" and 10.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.304 Olga 0 -0 0 13.5 0 0
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:29:29.00 +07:36:00.4: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:29:29.00 +07:36:00.4: 16.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 06 17.2502* 15 29 29.00 +07 36 00.4 13.3 U Ser 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461208.7502,13.33,0.05,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
VARIABLE_NAME 20260617.2502 13.33CV 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: 2461171.77913396 11.05.2026 06:41:47.174 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
First image: 2461171.77913396 11.05.2026 06:41:47.174 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
Last image: 2461208.75044529 17.06.2026 06:00:28.473 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 24
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 6659
Objects passed selection criteria: 6656
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 6625.75
Average stars matched: 6002.25 (90.5897 %)
Memory usage VmPeak: 113440 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 01:27:18 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: 2461171.77913396 11.05.2026 06:41:47.174 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
First image: 2461171.77913396 11.05.2026 06:41:47.174 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
Last image: 2461208.75044529 17.06.2026 06:00:28.473 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 97
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.01
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: 31 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): 41598
Objects passed selection criteria: 41531
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 44412.5
Average stars matched: 36363 (81.8756 %)
Memory usage VmPeak: 150508 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 01:30:05 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:
Ser-03-Q2b1x1
#######################################
########### Starting Ser-03-Q2b1x1 ###########
Processing Ser-03-Q2b1x1
WARNING: server tau is low on disk space, only 66458 MB free at /data_ssd/NMW-TexasTech/workdir
WARNING: server tau is low on disk space, only 66458 MB free at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
REFERENCE_EPOCH__SECOND_IMAGE= /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.png' -> 'transient_report/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits_preview.png'
Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
renamed 'Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.png' -> 'transient_report/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits_preview.png'
Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.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= 362.3371
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 480.6276
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 1029.9704
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 520.4843
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 1029.5200
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 521.8891
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 2.84258
INFO: SECOND_EPOCH__SD_ratio= 0.003
----------------------------------------------
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= 9.9 / [degC] CCD temperature
FOCTEMP = 26.0900001525879 / [degC] Focuser temperature
AMBTEMP = 26.4 / [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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
EXPTIME = 20.0 / [s] Exposure duration
SET-TEMP= 10.0 / [degC] CCD temperature setpoint
CCD-TEMP= 10.0 / [degC] CCD temperature
FOCTEMP = 25.7999992370605 / [degC] Focuser temperature
AMBTEMP = 26.4 / [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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
SECOND_EPOCH__SECOND_IMAGE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.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/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
SExtractor catalog cache: saved Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.cat to cache
SExtractor catalog cache: saved Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.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/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.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: 2461208.74991169
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_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits exists and is non-empty
Saving wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits to local_wcs_cache/
'wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits' -> 'local_wcs_cache/wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits'
wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits exists and is non-empty
Saving wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits to local_wcs_cache/
'wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits' -> 'local_wcs_cache/wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits'
wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits exists and is non-empty
Saving wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits to local_wcs_cache/
'wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits' -> 'local_wcs_cache/wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits'
wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits exists and is non-empty
Saving wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits to local_wcs_cache/
'wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits' -> 'local_wcs_cache/wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits (1st reference image)
verification OK: wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
Image size: 937.3'x624.2' 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: 15:25:43.591 +06:00:11.90 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits (1st new image)
verification OK: wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.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: 15:25:42.441 +06:00:10.27 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:25:43.591 +06:00:11.90
Second-epoch image center 15:25:42.441 +06:00:10.27
Angular distance between the image centers 0.0048 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits (2nd new image)
verification OK: wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.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: 15:25:44.978 +06:00:57.14 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:25:43.591 +06:00:11.90
Second-epoch image center 15:25:44.978 +06:00:57.14
Angular distance between the image centers 0.0138 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 15:25:42.441 +06:00:10.27
Second-epoch second image center 15:25:44.978 +06:00:57.14
Angular distance between the image centers 0.01673 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/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits &> /tmp/tmp.6H1ACG0fIP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits &> /tmp/tmp.CppV1LOocy
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits &> /tmp/tmp.WjMuxiWFcA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits &> /tmp/tmp.wIf5u72wSg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.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_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits and wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.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_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits and wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat
Found non-empty wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits and wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat
The reference image (wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits) and catalog (wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat) found
'wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat' -> 'wcsmag.cat'
Read 9347 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.4677 to 239.3571 deg, Dec +0.7206 to +11.2696 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 223.4677 to 239.3571 deg, Dec 0.7206 to 11.2696 deg
Loaded 4612 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): 3905 out of 4067 total matches.
Matched with Tycho-2 4067 out of 9347 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.701400
a=0.000000 b=1.000000 c=22.701400
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.39
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.39
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 9347 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.4677 to 239.3571 deg, Dec +0.7206 to +11.2696 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 223.4677 to 239.3571 deg, Dec 0.7206 to 11.2696 deg
Loaded 4612 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): 3905 out of 4067 total matches.
Matched with Tycho-2 4067 out of 9347 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits:
Forced-photometry filter: calibrated wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits -> calib.txt_param_ref_wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits (aperture=6.2)
Read 8606 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.4675 to 239.3569 deg, Dec +0.7513 to +11.2730 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 223.4675 to 239.3569 deg, Dec 0.7513 to 11.2730 deg
Loaded 4602 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): 3919 out of 4066 total matches.
Matched with Tycho-2 4066 out of 8606 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits:
Forced-photometry filter: calibrated wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits -> calib.txt_param_ref_wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits (aperture=6.1)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 24 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.3 pix Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
2.2 pix Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
2.2 pix Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
2.2 pix Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
2.3 pix wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
2.2 pix wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
Limiting magnitude estimates:
15.4 mag. Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
15.3 mag. Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
15.3 mag. Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
15.2 mag. Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
All-image limiting magnitude estimate: 15.2 (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.6H1ACG0fIP (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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits' -> 'wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
WCS_IMAGE_NAME=wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
WCS-calibrated image found: wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
Checking if the catalog wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat corresponding to the image wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits alredy exist and is non-empty...
Catalog wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat corresponding to the image wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
WCS catalog name: wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=545, passed=9347
Got 9347 stars (including 8797 good ones) from the SExtractor catalog wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat
util/solve_plate_with_UCAC5 got 9347 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 966 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 9164 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 973 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 9164 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Accuracy estimation diagnostic: 973 matched stars entering correct_measured_positions(), 9164 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 973 stars left (next iteration limit 1070)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits N_match=973 sigma_overall_arcsec=0.450 sigma_q1_arcsec=0.307 sigma_q2_arcsec=0.525 sigma_q3_arcsec=0.430 sigma_q4_arcsec=0.570 n_q1=210 n_q2=275 n_q3=216 n_q4=272 worst_quadrant_to_overall_ratio=1.268
The image catalog is written to wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits -region wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.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.CppV1LOocy (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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits' -> 'wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
WCS_IMAGE_NAME=wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
WCS-calibrated image found: wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
Checking if the catalog wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits.wcscat corresponding to the image wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits alredy exist and is non-empty...
Catalog wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits.wcscat corresponding to the image wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
WCS catalog name: wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=477, passed=8606
Got 8606 stars (including 8121 good ones) from the SExtractor catalog wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits.wcscat
util/solve_plate_with_UCAC5 got 8606 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 453 to 508 (Dec 0.8 to 11.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 8505 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
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 453 to 508 (Dec 0.8 to 11.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 8505 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 8505 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits N_match=975 sigma_overall_arcsec=0.438 sigma_q1_arcsec=0.339 sigma_q2_arcsec=0.671 sigma_q3_arcsec=0.374 sigma_q4_arcsec=0.576 n_q1=262 n_q2=237 n_q3=254 n_q4=222 worst_quadrant_to_overall_ratio=1.534
The image catalog is written to wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits -region wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.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.WjMuxiWFcA (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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
WCS_IMAGE_NAME=wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
WCS-calibrated image found: wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
Checking if the catalog wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits.wcscat corresponding to the image wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits alredy exist and is non-empty...
Catalog wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits.wcscat corresponding to the image wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
WCS catalog name: wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=514, passed=7813
Got 7813 stars (including 7294 good ones) from the SExtractor catalog wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits.wcscat
util/solve_plate_with_UCAC5 got 7813 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 7711 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 981 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 7708 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 981 matched stars entering correct_measured_positions(), 7708 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 981 stars left (next iteration limit 1079)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits N_match=981 sigma_overall_arcsec=0.402 sigma_q1_arcsec=0.322 sigma_q2_arcsec=0.596 sigma_q3_arcsec=0.325 sigma_q4_arcsec=0.491 n_q1=243 n_q2=271 n_q3=252 n_q4=215 worst_quadrant_to_overall_ratio=1.483
The image catalog is written to wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits -region wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.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.wIf5u72wSg (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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
WCS_IMAGE_NAME=wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
WCS-calibrated image found: wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
Checking if the catalog wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits.wcscat corresponding to the image wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits alredy exist and is non-empty...
Catalog wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits.wcscat corresponding to the image wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
WCS catalog name: wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=517, passed=7851
Got 7851 stars (including 7328 good ones) from the SExtractor catalog wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits.wcscat
util/solve_plate_with_UCAC5 got 7851 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 7739 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 7737 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 7737 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits N_match=979 sigma_overall_arcsec=0.396 sigma_q1_arcsec=0.322 sigma_q2_arcsec=0.566 sigma_q3_arcsec=0.347 sigma_q4_arcsec=0.476 n_q1=247 n_q2=265 n_q3=249 n_q4=218 worst_quadrant_to_overall_ratio=1.431
The image catalog is written to wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits -region wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.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=Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits sigma_overall=0.450 worst_q_ratio=1.268
ref2=Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits sigma_overall=0.438 worst_q_ratio=1.534
new1=Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits sigma_overall=0.402 worst_q_ratio=1.483
new2=Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits sigma_overall=0.396 worst_q_ratio=1.431
reference average sigma_overall=0.444 worst_q_ratio=1.401
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289_astrometric_residuals.png (973 matched stars from wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258_astrometric_residuals.png (975 matched stars from wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.39 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210_astrometric_residuals.png (981 matched stars from wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.36 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211_astrometric_residuals.png (979 matched stars from wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits'
Saving fully-calibrated image wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits'
Preparing the HTML report for the field Ser-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:28:39.12 +06:53:53.2: 12.34 +/- 0.01 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:26:21.11 +06:40:27.2: 12.61 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:25:56.27 +05:22:21.2: 12.57 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:17:58.11 +03:25:37.2: 12.34 +/- 0.01 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:28:29.13 +07:33:04.3: 12.61 +/- 0.01 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:27:53.07 +06:18:29.0: 12.54 +/- 0.01 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:23:33.23 +06:47:06.1: 12.49 +/- 0.01 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:28:39.12 +06:53:53.2: 12.36 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.35 +/- 0.01
Forced photometry filter REJECTED candidate at 15:28:39.12 +06:53:53.2: ref_mag=12.35 +/- 0.01 new_mean_mag=12.1849 delta=0.16 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:28:29.13 +07:33:04.3: 12.56 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:17:58.11 +03:25:37.2: 12.38 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter REJECTED candidate at 15:28:29.13 +07:33:04.3: ref_mag=12.59 +/- 0.01 new_mean_mag=12.4148 delta=0.17 (need > 0.90)
Forced photometry reference-image weighted average: 12.36 +/- 0.01
Forced photometry filter REJECTED candidate at 15:17:58.11 +03:25:37.2: ref_mag=12.36 +/- 0.01 new_mean_mag=12.4576 delta=-0.10 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:27:53.07 +06:18:29.0: 12.62 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:23:33.23 +06:47:06.1: 12.52 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 15:27:53.07 +06:18:29.0: ref_mag=12.57 +/- 0.01 new_mean_mag=12.4057 delta=0.16 (need > 0.90)
Forced photometry reference-image weighted average: 12.50 +/- 0.01
Forced photometry filter REJECTED candidate at 15:23:33.23 +06:47:06.1: ref_mag=12.50 +/- 0.01 new_mean_mag=12.3288 delta=0.17 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:24:10.70 +06:25:26.9: 12.61 +/- 0.01 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:26:21.11 +06:40:27.2: 12.63 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:25:56.27 +05:22:21.2: 12.54 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:31:34.05 +07:41:35.1: 12.56 +/- 0.01 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter REJECTED candidate at 15:26:21.11 +06:40:27.2: ref_mag=12.62 +/- 0.01 new_mean_mag=12.4187 delta=0.20 (need > 0.90)
Forced photometry reference-image weighted average: 12.55 +/- 0.01
Forced photometry filter REJECTED candidate at 15:25:56.27 +05:22:21.2: ref_mag=12.55 +/- 0.01 new_mean_mag=12.3944 delta=0.16 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:33:50.68 +07:07:26.6: 12.61 +/- 0.01 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:31:34.05 +07:41:35.1: 12.57 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:24:10.70 +06:25:26.9: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.57 +/- 0.01
Forced photometry filter REJECTED candidate at 15:31:34.05 +07:41:35.1: ref_mag=12.57 +/- 0.01 new_mean_mag=12.4210 delta=0.15 (need > 0.90)
Forced photometry reference-image weighted average: 12.60 +/- 0.01
Forced photometry filter REJECTED candidate at 15:24:10.70 +06:25:26.9: ref_mag=12.60 +/- 0.01 new_mean_mag=12.4298 delta=0.17 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:33:50.68 +07:07:26.6: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.61 +/- 0.01
Forced photometry filter REJECTED candidate at 15:33:50.68 +07:07:26.6: ref_mag=12.61 +/- 0.01 new_mean_mag=12.4624 delta=0.15 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:27:25.49 +05:13:17.6: 12.75 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:23:32.08 +05:17:16.9: 12.63 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:14:49.68 +06:37:39.0: 12.59 +/- 0.01 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:29:28.76 +07:25:28.1: 12.67 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:14:53.21 +05:50:58.6: 12.55 +/- 0.01 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:25:31.36 +05:07:55.2: 12.77 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:42:52.76 +06:03:38.6: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:23:32.08 +05:17:16.9: 12.67 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry filter REJECTED candidate at 15:23:32.08 +05:17:16.9: ref_mag=12.65 +/- 0.01 new_mean_mag=12.4713 delta=0.18 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:26:51.58 +05:19:45.6: 12.60 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:27:25.49 +05:13:17.6: 12.75 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.01
Forced photometry filter REJECTED candidate at 15:27:25.49 +05:13:17.6: ref_mag=12.75 +/- 0.01 new_mean_mag=12.4829 delta=0.26 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:14:53.21 +05:50:58.6: 12.62 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:14:49.68 +06:37:39.0: 12.59 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.58 +/- 0.01
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:29:28.76 +07:25:28.1: 12.63 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 15:14:53.21 +05:50:58.6: ref_mag=12.58 +/- 0.01 new_mean_mag=12.4763 delta=0.10 (need > 0.90)
Forced photometry reference-image weighted average: 12.65 +/- 0.01
Forced photometry reference-image weighted average: 12.59 +/- 0.01
Forced photometry filter REJECTED candidate at 15:29:28.76 +07:25:28.1: ref_mag=12.65 +/- 0.01 new_mean_mag=12.4881 delta=0.16 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:14:49.68 +06:37:39.0: ref_mag=12.59 +/- 0.01 new_mean_mag=12.4825 delta=0.11 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:30:59.76 +07:53:59.3: 12.61 +/- 0.01 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:42:52.76 +06:03:38.6: 15.78 +/- 99.00 upperlimit
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:25:31.36 +05:07:55.2: 12.76 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:23:58.44 +05:11:12.8: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.76 +/- 0.01
Forced photometry filter REJECTED candidate at 15:25:31.36 +05:07:55.2: ref_mag=12.76 +/- 0.01 new_mean_mag=12.5252 delta=0.24 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:26:51.58 +05:19:45.6: 12.68 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.64 +/- 0.01
Forced photometry filter REJECTED candidate at 15:26:51.58 +05:19:45.6: ref_mag=12.64 +/- 0.01 new_mean_mag=12.5061 delta=0.13 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:30:59.76 +07:53:59.3: 12.64 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.62 +/- 0.01
Forced photometry filter REJECTED candidate at 15:30:59.76 +07:53:59.3: ref_mag=12.62 +/- 0.01 new_mean_mag=12.5364 delta=0.09 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:23:58.44 +05:11:12.8: 12.70 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.70 +/- 0.01
Forced photometry filter REJECTED candidate at 15:23:58.44 +05:11:12.8: ref_mag=12.70 +/- 0.01 new_mean_mag=12.5408 delta=0.16 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:17:33.71 +06:32:35.2: 12.65 +/- 0.02 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:17:33.71 +06:32:35.2: 12.61 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.63 +/- 0.01
Forced photometry filter REJECTED candidate at 15:17:33.71 +06:32:35.2: ref_mag=12.63 +/- 0.01 new_mean_mag=12.5113 delta=0.12 (need > 0.90)
Adding exclusion_list_local.txt__out22243.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 9s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22214_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22214_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22217_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22217_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
**** FOUND 15:18:35.42 +02:06:30.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22224_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22224_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22227_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22227_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
**** FOUND 15:19:18.74 +07:53:06.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22228_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22228_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
**** FOUND 15:18:24.82 +02:02:03.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22229_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22229_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22230_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22230_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22231_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22231_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22232_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22232_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22233_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22233_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22234_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22234_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22235_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22235_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22237_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22237_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22238_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22238_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22239_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22239_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22240_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22240_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22241_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22241_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22242_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22242_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22243_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
Preparing report for the candidate 22243_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22244_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22244_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22245_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22245_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22246_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22246_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22248_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22248_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 22249_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 22249_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 11s
Prepared the HTML report for the field Ser-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 ####
15:42:52.76 +06:03:38.6
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/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
SExtractor catalog cache: saved Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.cat to cache
SExtractor catalog cache: saved Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
Creating symlink local_wcs_cache/wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
Creating symlink local_wcs_cache/wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
Creating symlink local_wcs_cache/wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.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_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits exists and is non-empty
wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits exists and is non-empty
wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits exists and is non-empty
wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits (1st reference image)
verification OK: wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
Image size: 937.3'x624.2' 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: 15:25:43.591 +06:00:11.90 J2000 4789.000 3195.000
###################################
The image scale is 5.87"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.8"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits (1st new image)
verification OK: wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.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: 15:25:42.441 +06:00:10.27 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 15:25:43.591 +06:00:11.90
Second-epoch image center 15:25:42.441 +06:00:10.27
Angular distance between the image centers 0.0048 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits (2nd new image)
verification OK: wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.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: 15:25:44.978 +06:00:57.14 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 15:25:43.591 +06:00:11.90
Second-epoch image center 15:25:44.978 +06:00:57.14
Angular distance between the image centers 0.0138 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 15:25:42.441 +06:00:10.27
Second-epoch second image center 15:25:44.978 +06:00:57.14
Angular distance between the image centers 0.01673 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/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits &> /tmp/tmp.Llse4nRJsP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits &> /tmp/tmp.2W4PCzW1o5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits &> /tmp/tmp.wzewZGJh0V
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits &> /tmp/tmp.nPXGEMuGyL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
Calibrating the magnitude scale
Found non-empty wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.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_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits and wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.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_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits and wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat
Found non-empty wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits and wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat
The reference image (wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits) and catalog (wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat) found
'wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat' -> 'wcsmag.cat'
Read 52266 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.4564 to 239.3740 deg, Dec +0.7180 to +11.2709 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 223.4564 to 239.3740 deg, Dec 0.7180 to 11.2709 deg
Loaded 4623 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): 3684 out of 4071 total matches.
Matched with Tycho-2 4071 out of 52266 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.577800
a=0.000000 b=1.000000 c=22.577800
From vast_summary.log: estimated ref. image limiting mag.: -7.01
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.57
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.57
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 52266 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.4564 to 239.3740 deg, Dec +0.7180 to +11.2709 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 223.4564 to 239.3740 deg, Dec 0.7180 to 11.2709 deg
Loaded 4623 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): 3684 out of 4071 total matches.
Matched with Tycho-2 4071 out of 52266 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits:
Forced-photometry filter: calibrated wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits -> calib.txt_param_ref_wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits (aperture=4.8)
Read 48109 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 223.4676 to 239.3758 deg, Dec +0.7481 to +11.2767 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 223.4676 to 239.3758 deg, Dec 0.7481 to 11.2767 deg
Loaded 4608 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): 3712 out of 4078 total matches.
Matched with Tycho-2 4078 out of 48109 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits:
Forced-photometry filter: calibrated wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits -> calib.txt_param_ref_wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits (aperture=4.8)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 37 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
2.2 pix Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
2.2 pix Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
2.2 pix Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
2.2 pix wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
2.2 pix wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
Limiting magnitude estimates:
15.6 mag. Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
15.4 mag. Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
15.5 mag. Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
15.5 mag. Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.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.Llse4nRJsP (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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits' -> 'wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
WCS_IMAGE_NAME=wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
WCS-calibrated image found: wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
Checking if the catalog wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat corresponding to the image wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits alredy exist and is non-empty...
Catalog wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat corresponding to the image wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits
WCS catalog name: wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=2645, passed=52251
Got 52251 stars (including 49541 good ones) from the SExtractor catalog wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat
util/solve_plate_with_UCAC5 got 52251 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 51531 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 51531 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Accuracy estimation diagnostic: 971 matched stars entering correct_measured_positions(), 51531 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 971 stars left (next iteration limit 1068)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits N_match=971 sigma_overall_arcsec=0.441 sigma_q1_arcsec=0.299 sigma_q2_arcsec=0.537 sigma_q3_arcsec=0.414 sigma_q4_arcsec=0.563 n_q1=221 n_q2=267 n_q3=218 n_q4=265 worst_quadrant_to_overall_ratio=1.276
The image catalog is written to wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits -region wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.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.2W4PCzW1o5 (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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits 571.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits' -> 'wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
WCS_IMAGE_NAME=wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
WCS-calibrated image found: wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
Checking if the catalog wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits.wcscat corresponding to the image wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits alredy exist and is non-empty...
Catalog wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits.wcscat corresponding to the image wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits
WCS catalog name: wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=9, blended=2468, passed=48100
Got 48100 stars (including 45575 good ones) from the SExtractor catalog wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits.wcscat
util/solve_plate_with_UCAC5 got 48100 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 961 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 47595 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 47596 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 47596 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits N_match=975 sigma_overall_arcsec=0.405 sigma_q1_arcsec=0.341 sigma_q2_arcsec=0.611 sigma_q3_arcsec=0.352 sigma_q4_arcsec=0.532 n_q1=268 n_q2=241 n_q3=253 n_q4=213 worst_quadrant_to_overall_ratio=1.509
The image catalog is written to wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits -region wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.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.wzewZGJh0V (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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
WCS_IMAGE_NAME=wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
WCS-calibrated image found: wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
Checking if the catalog wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits.wcscat corresponding to the image wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits alredy exist and is non-empty...
Catalog wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits.wcscat corresponding to the image wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
WCS catalog name: wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=2783, passed=56577
Got 56577 stars (including 53677 good ones) from the SExtractor catalog wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits.wcscat
util/solve_plate_with_UCAC5 got 56577 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 956 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 54795 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 979 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 54797 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 979 matched stars entering correct_measured_positions(), 54795 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 979 stars left (next iteration limit 1076)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits N_match=979 sigma_overall_arcsec=0.368 sigma_q1_arcsec=0.293 sigma_q2_arcsec=0.518 sigma_q3_arcsec=0.314 sigma_q4_arcsec=0.435 n_q1=255 n_q2=253 n_q3=262 n_q4=209 worst_quadrant_to_overall_ratio=1.411
The image catalog is written to wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits -region wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.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.nPXGEMuGyL (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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
WCS_IMAGE_NAME=wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
WCS-calibrated image found: wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
Checking if the catalog wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits.wcscat corresponding to the image wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits alredy exist and is non-empty...
Catalog wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits.wcscat corresponding to the image wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
WCS catalog name: wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=2888, passed=56405
Got 56405 stars (including 53392 good ones) from the SExtractor catalog wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits.wcscat
util/solve_plate_with_UCAC5 got 56405 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 955 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 54713 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 453 to 508 (Dec 0.7 to 11.3)
Done reading UCAC5 zone files...
Matched 977 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 54713 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 977 matched stars entering correct_measured_positions(), 54713 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 977 stars left (next iteration limit 1074)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits N_match=977 sigma_overall_arcsec=0.363 sigma_q1_arcsec=0.295 sigma_q2_arcsec=0.480 sigma_q3_arcsec=0.309 sigma_q4_arcsec=0.435 n_q1=268 n_q2=249 n_q3=251 n_q4=209 worst_quadrant_to_overall_ratio=1.323
The image catalog is written to wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits -region wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.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_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/wcs_Ser-03-Q2b1x1_2026-06-17_00-59-42_20.00sec_9.90C_LIGHT_0210.fits
Saving fully-calibrated image wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.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_Ser-03-Q2b1x1_012503_TTUQ2b1x1_2527489_uaXWfKku/wcs_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211.fits
Preparing the HTML report for the field Ser-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:27:50.57 +05:57:57.7: 14.67 +/- 0.09 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:35:06.79 +09:59:13.2: 14.62 +/- 0.09 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:28:25.30 +02:16:52.1: 14.49 +/- 0.08 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:37:28.35 +04:32:53.7: 14.86 +/- 0.10 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:41:44.00 +05:04:14.5: 14.84 +/- 0.11 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:43:04.25 +05:29:22.2: 14.67 +/- 0.09 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:43:39.48 +09:35:25.3: 14.33 +/- 0.07 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:39:07.97 +08:57:03.1: 14.74 +/- 0.10 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:10:49.53 +03:10:41.4: 14.39 +/- 0.08 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:21:24.14 +04:30:39.9: 14.77 +/- 0.10 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:28:25.30 +02:16:52.1: 14.42 +/- 0.09 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:10:49.53 +03:10:41.4: 14.27 +/- 0.07 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:41:44.00 +05:04:14.5: 14.89 +/- 0.14 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:21:24.14 +04:30:39.9: 14.66 +/- 0.10 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:39:07.97 +08:57:03.1: 14.60 +/- 0.10 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:43:39.48 +09:35:25.3: 14.70 +/- 0.11 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:37:28.35 +04:32:53.7: 14.93 +/- 0.13 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:35:06.79 +09:59:13.2: 14.51 +/- 0.09 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:27:50.57 +05:57:57.7: 14.70 +/- 0.10 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:43:04.25 +05:29:22.2: 14.58 +/- 0.10 detection
Forced photometry reference-image weighted average: 14.68 +/- 0.06
Forced photometry reference-image weighted average: 14.63 +/- 0.07
Forced photometry reference-image weighted average: 14.43 +/- 0.06
Forced photometry reference-image weighted average: 14.32 +/- 0.05
Forced photometry reference-image weighted average: 14.57 +/- 0.06
Forced photometry reference-image weighted average: 14.72 +/- 0.07
Forced photometry reference-image weighted average: 14.86 +/- 0.09
Forced photometry reference-image weighted average: 14.67 +/- 0.07
Forced photometry reference-image weighted average: 14.88 +/- 0.08
Forced photometry reference-image weighted average: 14.46 +/- 0.06
Forced photometry filter REJECTED candidate at 15:41:44.00 +05:04:14.5: ref_mag=14.86 +/- 0.09 new_mean_mag=14.9716 delta=-0.11 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:28:25.30 +02:16:52.1: ref_mag=14.46 +/- 0.06 new_mean_mag=14.4100 delta=0.05 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:39:07.97 +08:57:03.1: ref_mag=14.67 +/- 0.07 new_mean_mag=14.9166 delta=-0.24 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:35:06.79 +09:59:13.2: ref_mag=14.57 +/- 0.06 new_mean_mag=14.7141 delta=-0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:27:50.57 +05:57:57.7: ref_mag=14.68 +/- 0.06 new_mean_mag=14.5259 delta=0.15 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:21:24.14 +04:30:39.9: ref_mag=14.72 +/- 0.07 new_mean_mag=14.7415 delta=-0.02 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:10:49.53 +03:10:41.4: ref_mag=14.32 +/- 0.05 new_mean_mag=14.3886 delta=-0.07 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:37:28.35 +04:32:53.7: ref_mag=14.88 +/- 0.08 new_mean_mag=14.7956 delta=0.09 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:43:04.25 +05:29:22.2: ref_mag=14.63 +/- 0.07 new_mean_mag=14.8055 delta=-0.18 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:43:39.48 +09:35:25.3: ref_mag=14.43 +/- 0.06 new_mean_mag=14.6953 delta=-0.27 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:10:49.97 +04:23:24.5: 13.45 +/- 0.03 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:15:03.93 +03:43:45.3: 13.38 +/- 0.03 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:12:28.49 +09:59:37.6: 13.79 +/- 0.04 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:19:19.61 +01:52:17.4: 16.12 +/- 99.00 upperlimit
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:30:04.82 +10:06:49.6: 13.95 +/- 0.05 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:24:19.92 +09:34:20.1: 14.26 +/- 0.06 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:40:38.48 +08:16:26.0: 13.83 +/- 0.04 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:18:57.46 +02:27:52.9: 13.31 +/- 0.03 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:31:42.47 +06:27:58.1: 12.03 +/- 0.01 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:29:29.00 +07:36:00.4: 16.18 +/- 99.00 upperlimit
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:12:28.49 +09:59:37.6: 14.03 +/- 0.05 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:15:03.93 +03:43:45.3: 13.54 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.87 +/- 0.03
Forced photometry reference-image weighted average: 13.44 +/- 0.02
Forced photometry filter REJECTED candidate at 15:12:28.49 +09:59:37.6: ref_mag=13.87 +/- 0.03 new_mean_mag=14.2463 delta=-0.37 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:15:03.93 +03:43:45.3: ref_mag=13.44 +/- 0.02 new_mean_mag=13.4607 delta=-0.02 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:30:04.82 +10:06:49.6: 14.04 +/- 0.06 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:10:49.97 +04:23:24.5: 13.59 +/- 0.04 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:19:19.61 +01:52:17.4: 15.95 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.51 +/- 0.02
Forced photometry reference-image weighted average: 13.98 +/- 0.04
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:40:38.48 +08:16:26.0: 13.77 +/- 0.05 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:24:19.92 +09:34:20.1: 14.15 +/- 0.06 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:18:57.46 +02:27:52.9: 13.33 +/- 0.03 detection
Forced photometry filter REJECTED candidate at 15:10:49.97 +04:23:24.5: ref_mag=13.51 +/- 0.02 new_mean_mag=13.7287 delta=-0.22 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:30:04.82 +10:06:49.6: ref_mag=13.98 +/- 0.04 new_mean_mag=14.3748 delta=-0.39 (need > 0.90)
Forced photometry reference-image weighted average: 13.80 +/- 0.03
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:31:42.47 +06:27:58.1: 12.00 +/- 0.01 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:29:29.00 +07:36:00.4: 16.04 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Forced photometry filter REJECTED candidate at 15:40:38.48 +08:16:26.0: ref_mag=13.80 +/- 0.03 new_mean_mag=13.9018 delta=-0.10 (need > 0.90)
Forced photometry reference-image weighted average: 14.20 +/- 0.04
Forced photometry filter REJECTED candidate at 15:18:57.46 +02:27:52.9: ref_mag=13.32 +/- 0.02 new_mean_mag=13.3943 delta=-0.08 (need > 0.90)
Forced photometry reference-image weighted average: 12.02 +/- 0.01
Forced photometry filter REJECTED candidate at 15:31:42.47 +06:27:58.1: ref_mag=12.02 +/- 0.01 new_mean_mag=11.8742 delta=0.14 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:24:19.92 +09:34:20.1: ref_mag=14.20 +/- 0.04 new_mean_mag=14.4516 delta=-0.25 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:33:47.81 +05:17:30.9: 14.42 +/- 0.07 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:18:29.45 +02:07:41.6: 13.22 +/- 0.08 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:18:29.45 +02:07:41.6: 13.34 +/- 0.09 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:33:47.81 +05:17:30.9: 14.42 +/- 0.08 detection
Forced photometry reference-image weighted average: 13.28 +/- 0.06
Forced photometry reference-image weighted average: 14.42 +/- 0.05
Forced photometry filter REJECTED candidate at 15:33:47.81 +05:17:30.9: ref_mag=14.42 +/- 0.05 new_mean_mag=14.3942 delta=0.03 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:09:51.33 +04:00:45.3: 14.82 +/- 0.12 detection
Forced photometry filter REJECTED candidate at 15:18:29.45 +02:07:41.6: ref_mag=13.28 +/- 0.06 new_mean_mag=13.3952 delta=-0.12 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:22:26.41 +03:31:16.2: 14.38 +/- 0.08 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:11:02.50 +01:52:05.8: 15.09 +/- 0.17 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:42:25.97 +03:39:25.3: 15.06 +/- 0.14 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:12:47.51 +07:26:02.7: 15.12 +/- 0.16 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:09:51.33 +04:00:45.3: 14.93 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.86 +/- 0.09
Forced photometry filter REJECTED candidate at 15:09:51.33 +04:00:45.3: ref_mag=14.86 +/- 0.09 new_mean_mag=14.6285 delta=0.23 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:33:09.81 +03:36:55.2: 15.19 +/- 0.15 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:22:26.41 +03:31:16.2: 14.41 +/- 0.09 detection
Forced photometry reference-image weighted average: 14.39 +/- 0.06
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:11:02.50 +01:52:05.8: 14.99 +/- 0.17 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:42:25.97 +03:39:25.3: 15.14 +/- 0.18 detection
Forced photometry filter REJECTED candidate at 15:22:26.41 +03:31:16.2: ref_mag=14.39 +/- 0.06 new_mean_mag=14.5036 delta=-0.11 (need > 0.90)
Forced photometry reference-image weighted average: 15.09 +/- 0.11
Forced photometry reference-image weighted average: 15.04 +/- 0.12
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:12:47.51 +07:26:02.7: 15.30 +/- 0.20 detection
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:33:09.81 +03:36:55.2: 15.14 +/- 0.16 detection
Forced photometry filter REJECTED candidate at 15:11:02.50 +01:52:05.8: ref_mag=15.04 +/- 0.12 new_mean_mag=14.8479 delta=0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:42:25.97 +03:39:25.3: ref_mag=15.09 +/- 0.11 new_mean_mag=14.9154 delta=0.18 (need > 0.90)
Forced photometry reference-image weighted average: 15.19 +/- 0.12
Forced photometry reference-image weighted average: 15.17 +/- 0.11
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-11_01-41-47_20.00sec_-5.00C_LIGHT_0289.fits at 15:39:46.49 +05:47:20.1: 14.99 +/- 0.12 detection
Forced photometry filter REJECTED candidate at 15:12:47.51 +07:26:02.7: ref_mag=15.19 +/- 0.12 new_mean_mag=14.9228 delta=0.27 (need > 0.90)
Forced photometry filter REJECTED candidate at 15:33:09.81 +03:36:55.2: ref_mag=15.17 +/- 0.11 new_mean_mag=14.8983 delta=0.27 (need > 0.90)
Forced photometry on wcs_Ser-03-Q2b1x1_2026-05-12_02-08-33_20.00sec_-4.90C_LIGHT_0258.fits at 15:39:46.49 +05:47:20.1: 14.98 +/- 0.14 detection
Forced photometry reference-image weighted average: 14.99 +/- 0.09
Forced photometry filter REJECTED candidate at 15:39:46.49 +05:47:20.1: ref_mag=14.99 +/- 0.09 new_mean_mag=14.9405 delta=0.05 (need > 0.90)
Adding exclusion_list_local.txt__out75616.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75876.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 10s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75008_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75008_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75014_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75014_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75029_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75029_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75034_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75034_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75037_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75037_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75039_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75039_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75043_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75043_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75045_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75045_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75048_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75048_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75053_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75053_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75054_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75054_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75059_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75059_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75061_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75061_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75067_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75067_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75070_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75070_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75073_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75073_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75074_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75074_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75076_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75076_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75451_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 75451_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
**** FOUND 15:42:52.75 +06:03:38.6 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75616_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
Preparing report for the candidate 75616_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 75876_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
Preparing report for the candidate 75876_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76014_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 76014_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77471_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 77471_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77527_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 77527_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
Rejecting candidate due to large distance (15.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77575_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 77575_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77679_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 77679_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78112_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 78112_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 78742_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 78742_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79126_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 79126_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79275_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 79275_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79318_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 79318_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79474_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 79474_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79861_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 79861_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79873_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 79873_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80273_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 80273_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80324_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 80324_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 80552_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211
The candidate 80552_Ser-03-Q2b1x1_2026-06-17_01-00-28_20.00sec_10.00C_LIGHT_0211 did not pass the final checks
