This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF
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 18.1336 2461209.6336 12.29 08:54:18.56 +20:15:03.7
206.59771 35.75673 galactic Cnc Second-epoch detections are separated by 0.2" and 3.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.40 Harmonia -0 0 0 11.7 0 -0
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 08:54:18.56 +20:15:03.7: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 08:54:18.56 +20:15:03.7: 16.13 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461209.6336,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260618.1336 12.29CV 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 18.1336 2461209.6336 14.74 08:44:48.97 +19:40:54.3
206.33055 33.46514 galactic Cnc Second-epoch detections are separated by 7.9" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:44:48.97 +19:40:54.3 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 08:44:48.97 +19:40:54.3: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 08:44:48.97 +19:40:54.3: 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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461209.6336,14.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260618.1336 14.74CV 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 18.1336 2461209.6336 14.59 08:44:42.33 +19:45:43.6
206.22935 33.46831 galactic Cnc Second-epoch detections are separated by 5.5" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:44:42.33 +19:45:43.6 (user input) | T | P | (position from user input)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 08:44:42.33 +19:45:43.6: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 08:44:42.33 +19:45:43.6: 16.01 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461209.6336,14.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260618.1336 14.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.71707330 22.02.2026 05:12:25.133 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
First image: 2461093.71707330 22.02.2026 05:12:25.133 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Last image: 2461209.63380691 18.06.2026 03:12:30.917 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 1
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.54
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 8661
Objects passed selection criteria: 8618
Measurements per detected object (mean, median, min, max): 2.6 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.6 2.0 2 4
Average stars detected per image: 5914.5
Average stars matched: 5743.5 (97.1088 %)
Memory usage VmPeak: 114352 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 22:15:38 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461093.71707330 22.02.2026 05:12:25.133 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
First image: 2461093.71707330 22.02.2026 05:12:25.133 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Last image: 2461209.63380691 18.06.2026 03:12:30.917 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 22
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
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: 10 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): 47388
Objects passed selection criteria: 47227
Measurements per detected object (mean, median, min, max): 2.7 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.7 2.0 2 4
Average stars detected per image: 33846.5
Average stars matched: 32600.5 (96.3187 %)
Memory usage VmPeak: 148484 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 22:17:20 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.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: 2461209.63336672
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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits exists and is non-empty
Saving wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits to local_wcs_cache/
'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits'
wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits exists and is non-empty
Saving wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits to local_wcs_cache/
'wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits' -> 'local_wcs_cache/wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits'
wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits'
wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits exists and is non-empty
Saving wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits to local_wcs_cache/
'wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits' -> 'local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (1st reference image)
verification OK: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:13:50.749 +22:00:00.30 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits (1st new image)
verification OK: wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
Image size: 941.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:14:00.330 +22:01:08.23 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:13:50.749 +22:00:00.30
Second-epoch image center 09:14:00.330 +22:01:08.23
Angular distance between the image centers 0.0415 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits (2nd new image)
verification OK: wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
Image size: 941.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:14:00.474 +22:01:30.11 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:13:50.749 +22:00:00.30
Second-epoch image center 09:14:00.474 +22:01:30.11
Angular distance between the image centers 0.0451 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 09:14:00.330 +22:01:08.23
Second-epoch second image center 09:14:00.474 +22:01:30.11
Angular distance between the image centers 0.00610 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/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits &> /tmp/tmp.QvgozdLB5y
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits &> /tmp/tmp.FAjfi9vfus
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits &> /tmp/tmp.EMYycXSXZc
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits &> /tmp/tmp.VnwBmOkrso
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
Found non-empty wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
The reference image (wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits) and catalog (wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat) found
'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat' -> 'wcsmag.cat'
Read 9058 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4948 to 147.0574 deg, Dec +16.3332 to +27.3468 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 129.4948 to 147.0574 deg, Dec 16.3332 to 27.3468 deg
Loaded 6004 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): 4516 out of 4805 total matches.
Matched with Tycho-2 4805 out of 9058 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.920350
a=0.000000 b=1.000000 c=22.920350
From vast_summary.log: estimated ref. image limiting mag.: -7.54
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.38
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.38
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 9058 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4948 to 147.0574 deg, Dec +16.3332 to +27.3468 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 129.4948 to 147.0574 deg, Dec 16.3332 to 27.3468 deg
Loaded 6004 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): 4516 out of 4805 total matches.
Matched with Tycho-2 4805 out of 9058 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits:
Forced-photometry filter: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits -> calib.txt_param_ref_wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (aperture=6.3)
Read 9037 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4948 to 147.0612 deg, Dec +16.3333 to +27.3527 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 129.4948 to 147.0612 deg, Dec 16.3333 to 27.3527 deg
Loaded 6007 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): 4487 out of 4795 total matches.
Matched with Tycho-2 4795 out of 9037 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits:
Forced-photometry filter: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits -> calib.txt_param_ref_wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits (aperture=6.3)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.2 pix Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
2.2 pix Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
2.4 pix fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
2.4 pix fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
2.2 pix wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
2.2 pix wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Limiting magnitude estimates:
15.4 mag. Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
15.4 mag. Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
13.8 mag. fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
13.8 mag. fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
All-image limiting magnitude estimate: 13.8 (SNR ) 10.9 (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.QvgozdLB5y (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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits' -> 'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=691, passed=9058
Got 9058 stars (including 8360 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
util/solve_plate_with_UCAC5 got 9058 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 8974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 8975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 8975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits N_match=957 sigma_overall_arcsec=0.381 sigma_q1_arcsec=0.455 sigma_q2_arcsec=0.400 sigma_q3_arcsec=0.362 sigma_q4_arcsec=0.337 n_q1=266 n_q2=204 n_q3=249 n_q4=238 worst_quadrant_to_overall_ratio=1.194
The image catalog is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits -region wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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.FAjfi9vfus (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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits' -> 'wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=724, passed=9037
Got 9037 stars (including 8310 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat
util/solve_plate_with_UCAC5 got 9037 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 8949 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 8948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 8948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits N_match=958 sigma_overall_arcsec=0.407 sigma_q1_arcsec=0.483 sigma_q2_arcsec=0.443 sigma_q3_arcsec=0.392 sigma_q4_arcsec=0.345 n_q1=262 n_q2=201 n_q3=256 n_q4=239 worst_quadrant_to_overall_ratio=1.185
The image catalog is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits -region wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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.EMYycXSXZc (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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=312, passed=2830
Got 2830 stars (including 2516 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits.wcscat
util/solve_plate_with_UCAC5 got 2830 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 589 (Dec 16.3 to 27.5)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 931 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 2732 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 531 to 589 (Dec 16.3 to 27.5)
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 2734 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 951 matched stars entering correct_measured_positions(), 2734 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits N_match=951 sigma_overall_arcsec=0.316 sigma_q1_arcsec=0.312 sigma_q2_arcsec=0.357 sigma_q3_arcsec=0.248 sigma_q4_arcsec=0.338 n_q1=165 n_q2=285 n_q3=199 n_q4=302 worst_quadrant_to_overall_ratio=1.129
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.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.VnwBmOkrso (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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=335, passed=2998
Got 2998 stars (including 2658 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat
util/solve_plate_with_UCAC5 got 2998 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 589 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 2890 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 531 to 589 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 2886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 2886 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits N_match=953 sigma_overall_arcsec=0.320 sigma_q1_arcsec=0.316 sigma_q2_arcsec=0.368 sigma_q3_arcsec=0.241 sigma_q4_arcsec=0.366 n_q1=175 n_q2=285 n_q3=203 n_q4=290 worst_quadrant_to_overall_ratio=1.149
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.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=Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits sigma_overall=0.381 worst_q_ratio=1.194
ref2=Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits sigma_overall=0.407 worst_q_ratio=1.185
new1=fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits sigma_overall=0.316 worst_q_ratio=1.129
new2=fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits sigma_overall=0.320 worst_q_ratio=1.149
reference average sigma_overall=0.394 worst_q_ratio=1.1895
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199_astrometric_residuals.png (957 matched stars from wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.35 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200_astrometric_residuals.png (958 matched stars from wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.37 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022_astrometric_residuals.png (951 matched stars from wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023_astrometric_residuals.png (953 matched stars from wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.30 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits'
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits'
Preparing the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20568_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 20568_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 09:43:25.53 +19:51:39.4 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.cat to cache
SExtractor catalog cache: saved Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Creating symlink local_wcs_cache/wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits exists and is non-empty
wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits exists and is non-empty
wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits exists and is non-empty
wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (1st reference image)
verification OK: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Image size: 941.6'x627.1' 15.7(deg)x10.5(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:13:50.749 +22:00:00.30 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits (1st new image)
verification OK: wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
Image size: 941.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:14:00.330 +22:01:08.23 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 09:13:50.749 +22:00:00.30
Second-epoch image center 09:14:00.330 +22:01:08.23
Angular distance between the image centers 0.0415 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits (2nd new image)
verification OK: wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
Image size: 941.7'x626.7' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 09:14:00.474 +22:01:30.11 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 09:13:50.749 +22:00:00.30
Second-epoch image center 09:14:00.474 +22:01:30.11
Angular distance between the image centers 0.0451 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 09:14:00.330 +22:01:08.23
Second-epoch second image center 09:14:00.474 +22:01:30.11
Angular distance between the image centers 0.00610 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/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits &> /tmp/tmp.VirR581oAi
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits &> /tmp/tmp.ndouCbBqIx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits &> /tmp/tmp.D7zspZXzQ7
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits &> /tmp/tmp.APwzf4i3P3
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
Found non-empty wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits and wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
The reference image (wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits) and catalog (wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat) found
'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat' -> 'wcsmag.cat'
Read 50507 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4949 to 147.0725 deg, Dec +16.3332 to +27.3504 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 129.4949 to 147.0725 deg, Dec 16.3332 to 27.3504 deg
Loaded 6013 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): 4206 out of 4845 total matches.
Matched with Tycho-2 4845 out of 50507 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.814650
a=0.000000 b=1.000000 c=22.814650
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.52
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.52
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 50507 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4949 to 147.0725 deg, Dec +16.3332 to +27.3504 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 129.4949 to 147.0725 deg, Dec 16.3332 to 27.3504 deg
Loaded 6013 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): 4206 out of 4845 total matches.
Matched with Tycho-2 4845 out of 50507 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits:
Forced-photometry filter: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits -> calib.txt_param_ref_wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits (aperture=5.0)
Read 50709 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 129.4922 to 147.0612 deg, Dec +16.3288 to +27.3568 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 129.4922 to 147.0612 deg, Dec 16.3288 to 27.3568 deg
Loaded 6019 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): 4180 out of 4844 total matches.
Matched with Tycho-2 4844 out of 50709 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits:
Forced-photometry filter: calibrated wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits -> calib.txt_param_ref_wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 21 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
2.0 pix Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
2.2 pix fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
2.2 pix fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
2.0 pix wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
2.0 pix wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Limiting magnitude estimates:
15.5 mag. Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
15.5 mag. Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
15.6 mag. fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
15.5 mag. fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 13.4 (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.VirR581oAi (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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits' -> 'wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=2848, passed=50482
Got 50482 stars (including 47533 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat
util/solve_plate_with_UCAC5 got 50482 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 948 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 50087 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 531 to 588 (Dec 16.3 to 27.3)
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 50084 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 953 matched stars entering correct_measured_positions(), 50083 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits N_match=953 sigma_overall_arcsec=0.385 sigma_q1_arcsec=0.440 sigma_q2_arcsec=0.394 sigma_q3_arcsec=0.362 sigma_q4_arcsec=0.354 n_q1=260 n_q2=193 n_q3=256 n_q4=244 worst_quadrant_to_overall_ratio=1.144
The image catalog is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits -region wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.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.ndouCbBqIx (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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits' -> 'wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS_IMAGE_NAME=wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS-calibrated image found: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
Checking if the catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits alredy exist and is non-empty...
Catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat corresponding to the image wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits
WCS catalog name: wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=29, blended=2904, passed=50680
Got 50680 stars (including 47694 good ones) from the SExtractor catalog wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat
util/solve_plate_with_UCAC5 got 50680 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 946 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 50198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 531 to 588 (Dec 16.3 to 27.4)
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 50198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Accuracy estimation diagnostic: 957 matched stars entering correct_measured_positions(), 50198 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.42"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits N_match=957 sigma_overall_arcsec=0.416 sigma_q1_arcsec=0.470 sigma_q2_arcsec=0.403 sigma_q3_arcsec=0.394 sigma_q4_arcsec=0.376 n_q1=259 n_q2=193 n_q3=261 n_q4=244 worst_quadrant_to_overall_ratio=1.130
The image catalog is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits -region wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.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.D7zspZXzQ7 (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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=10, blended=631, passed=17276
Got 17276 stars (including 16617 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits.wcscat
util/solve_plate_with_UCAC5 got 17276 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 938 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 16923 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 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 16923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 955 matched stars entering correct_measured_positions(), 16923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits N_match=955 sigma_overall_arcsec=0.333 sigma_q1_arcsec=0.336 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.279 sigma_q4_arcsec=0.329 n_q1=167 n_q2=279 n_q3=197 n_q4=312 worst_quadrant_to_overall_ratio=1.070
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.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.APwzf4i3P3 (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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
WCS-calibrated image found: wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
Checking if the catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat corresponding to the image wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
WCS catalog name: wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=1, no_mag_err=0, low_SNR=6, blended=661, passed=17863
Got 17863 stars (including 17175 good ones) from the SExtractor catalog wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat
util/solve_plate_with_UCAC5 got 17863 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 937 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 17475 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 530 to 589 (Dec 16.2 to 27.5)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 17475 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 17475 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
WCS_QUALITY_DIAG: file=fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits N_match=956 sigma_overall_arcsec=0.333 sigma_q1_arcsec=0.325 sigma_q2_arcsec=0.382 sigma_q3_arcsec=0.251 sigma_q4_arcsec=0.357 n_q1=179 n_q2=278 n_q3=204 n_q4=295 worst_quadrant_to_overall_ratio=1.147
The image catalog is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-06-17_CI_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits -region wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.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_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-11-52_20.00sec_0.00C_LIGHTs_0022.fits
Saving fully-calibrated image wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.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_Cnc-03-Q1b1x1_221324_TTUQ1b1x1_906347_VQzyDLMF/wcs_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023.fits
Preparing the HTML report for the field Cnc-03-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:06:55.90 +22:23:19.3: 13.02 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:09:13.13 +22:04:11.8: 12.89 +/- 0.02 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 08:54:18.56 +20:15:03.7: 16.13 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 09:04:51.13 +24:37:35.1: 13.34 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 08:44:48.97 +19:40:54.3: 15.96 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-12-25_20.00sec_-15.00C_LIGHT_0199.fits at 08:44:42.33 +19:45:43.6: 16.01 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:09:13.13 +22:04:11.8: 12.91 +/- 0.02 detection
Forced photometry reference-image weighted average: 12.90 +/- 0.01
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:06:55.90 +22:23:19.3: 13.03 +/- 0.02 detection
Forced photometry filter REJECTED candidate at 09:09:13.13 +22:04:11.8: ref_mag=12.90 +/- 0.01 new_mean_mag=12.7116 delta=0.19 (need > 0.90)
Forced photometry reference-image weighted average: 13.02 +/- 0.02
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 08:54:18.56 +20:15:03.7: 16.13 +/- 99.00 upperlimit
Forced photometry filter REJECTED candidate at 09:06:55.90 +22:23:19.3: ref_mag=13.02 +/- 0.02 new_mean_mag=12.8976 delta=0.13 (need > 0.90)
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 08:44:48.97 +19:40:54.3: 15.95 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 09:04:51.13 +24:37:35.1: 13.31 +/- 0.03 detection
Forced photometry on wcs_Cnc-03-Q1b1x1_2026-02-21_23-13-17_20.00sec_-15.00C_LIGHT_0200.fits at 08:44:42.33 +19:45:43.6: 16.01 +/- 99.00 upperlimit
Forced photometry reference-image weighted average: 13.32 +/- 0.02
Forced photometry filter REJECTED candidate at 09:04:51.13 +24:37:35.1: ref_mag=13.32 +/- 0.02 new_mean_mag=13.1666 delta=0.16 (need > 0.90)
Adding exclusion_list_local.txt__out64490.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out65039.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 2s
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Considering the candidate 64490_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 64490_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
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Considering the candidate 64536_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 64536_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 09:37:50.55 +16:59:19.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64601_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 64601_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
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Considering the candidate 64627_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 64627_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 09:19:28.93 +25:10:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64663_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 64663_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
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Considering the candidate 64665_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 64665_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 09:05:00.96 +22:48:38.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64674_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 64674_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 09:09:54.00 +25:12:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64763_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 64763_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 09:16:16.58 +23:25:03.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64779_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 64779_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 09:04:57.36 +24:36:57.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64781_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 64781_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 08:54:55.80 +26:13:12.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64846_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 64846_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
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Considering the candidate 64905_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 64905_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 09:20:35.12 +22:39:16.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64934_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 64934_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 09:11:24.14 +23:05:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 64978_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 64978_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 09:09:47.17 +25:13:35.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 65032_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 65032_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 65038_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 65038_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
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Considering the candidate 65039_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
Preparing report for the candidate 65039_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
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Considering the candidate 65040_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 65040_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 14155_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 14155_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 09:43:25.50 +19:51:39.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39522_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 39522_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks
**** FOUND 08:51:19.59 +25:33:24.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 13343_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023
The candidate 13343_fd_Cnc-03-Q1b1x1_2026-06-17_22-12-30_20.00sec_-0.00C_LIGHTs_0023 did not pass the final checks