This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi
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 09 07.4478 2461290.9478 10.72 08:28:41.46 +13:28:27.1
211.32890 27.55451 galactic Cnc Second-epoch detections are separated by 0.9" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.6 Hebe 0 0 0 10.7 0 0
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits at 08:28:41.46 +13:28:27.1: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits at 08:28:41.46 +13:28:27.1: 15.69 +/- 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,2461290.9478,10.72,0.05,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 20260907.4478 10.72CV 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 09 07.4478 2461290.9478 12.68 08:17:09.06 +14:04:28.2
209.45606 25.23119 galactic Cnc Second-epoch detections are separated by 2.1" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.12 Victoria 1 2 2 13.1 0 0
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits at 08:17:09.06 +14:04:28.2: 15.88 +/- 0.30 detection
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits at 08:17:09.06 +14:04:28.2: 15.17 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.33 +/- 0.15
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,2461290.9478,12.68,0.05,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 20260907.4478 12.68CV 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 09 07.4478 2461290.9478 13.33 07:36:02.46 +11:40:14.5
207.36374 15.11737 galactic CMi Second-epoch detections are separated by 1.1" and 8.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.85 Io -0 -1 1 13.8 0 0
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits at 07:36:02.46 +11:40:14.5: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits at 07:36:02.46 +11:40:14.5: 15.87 +/- 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,2461290.9478,13.33,0.05,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 20260907.4478 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
Mean magnitude and position on the discovery images:
2026 09 07.4478 2461290.9478 13.92 07:46:38.78 +17:11:32.9
203.19821 19.73177 galactic Gem Second-epoch detections are separated by 2.5" and 8.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.405 Thia 0 -1 1 14.2 -0 0
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits at 07:46:38.78 +17:11:32.9: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits at 07:46:38.78 +17:11:32.9: 15.94 +/- 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,2461290.9478,13.92,0.05,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 20260907.4478 13.92CV 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 09 07.4478 2461290.9478 13.04 07:44:10.10 +16:39:28.0
203.46786 18.97518 galactic Gem Second-epoch detections are separated by 0.2" and 9.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was found in astcheck.202 Chryseis 0 -0 0 13.4 0 0
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits at 07:44:10.10 +16:39:28.0: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits at 07:44:10.10 +16:39:28.0: 16.04 +/- 99.00 upperlimit
Check this position in TNS.Manually check the ASAS-SN list of transients!Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
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,2461290.9478,13.04,0.05,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 20260907.4478 13.04CV 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: 2461093.69369509 22.02.2026 04:38:45.256 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
First image: 2461093.69369509 22.02.2026 04:38:45.256 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
Last image: 2461290.94812397 07.09.2026 10:45:07.911 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.60
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: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 16633
Objects passed selection criteria: 16596
Measurements per detected object (mean, median, min, max): 3.0 3.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 3.0 2 4
Average stars detected per image: 13023.8
Average stars matched: 12527 (96.1858 %)
Memory usage VmPeak: 242032 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Sep 7 05:48:06 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: 2461093.69369509 22.02.2026 04:38:45.256 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
First image: 2461093.69369509 22.02.2026 04:38:45.256 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
Last image: 2461290.94812397 07.09.2026 10:45:07.911 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 50
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: 22 seconds
Number of parallel threads: 3
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
VAST_SKIP_INDEX_VS_MAG is set - skipping the lib/index_vs_mag variability-index fitting
Total objects detected (at least 2 times): 103998
Objects passed selection criteria: 103755
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 79421.2
Average stars matched: 77336.5 (97.3751 %)
Memory usage VmPeak: 568472 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Wed Sep 2 15:05:04 CDT 2026
VaST build number 1.0rc89-201-ga7d4d23b
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-09-02)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Sep 7 05:49:12 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 --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
SExtractor catalog cache: saved Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.cat to cache
SExtractor catalog cache: saved Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.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-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.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: 2461290.94752146
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-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits exists and is non-empty
wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits exists and is non-empty
wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits exists and is non-empty
wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits (1st reference image)
verification OK: wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
Image size: 941.7'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: 07:59:57.821 +13:59:32.16 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-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits (1st new image)
verification OK: wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
Image size: 942.8'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:59:55.719 +13:56:52.81 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:59:57.821 +13:59:32.16
Second-epoch image center 07:59:55.719 +13:56:52.81
Angular distance between the image centers 0.0451 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits (2nd new image)
verification OK: wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
Image size: 942.7'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:59:58.694 +13:56:21.74 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:59:57.821 +13:59:32.16
Second-epoch image center 07:59:58.694 +13:56:21.74
Angular distance between the image centers 0.0530 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 07:59:55.719 +13:56:52.81
Second-epoch second image center 07:59:58.694 +13:56:21.74
Angular distance between the image centers 0.01481 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits &> /tmp/tmp.mHeROAkPRl
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits &> /tmp/tmp.7ykIFEkrxu
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits &> /tmp/tmp.Gddba4zqmW
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits &> /tmp/tmp.GZ1MtmHB5w
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.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-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits and wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.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-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits and wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat
Found non-empty wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits and wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat
The reference image (wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits) and catalog (wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat) found
'wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat' -> 'wcsmag.cat'
Read 17766 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 111.5759 to 128.1392 deg, Dec +8.4757 to +19.3219 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 111.5759 to 128.1392 deg, Dec 8.4757 to 19.3219 deg
Loaded 10985 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): 8491 out of 9314 total matches.
Matched with Tycho-2 9314 out of 17766 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.911300
a=0.000000 b=1.000000 c=22.911300
From vast_summary.log: estimated ref. image limiting mag.: -7.60
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.31
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.31
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 17766 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 111.5759 to 128.1392 deg, Dec +8.4757 to +19.3219 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 111.5759 to 128.1392 deg, Dec 8.4757 to 19.3219 deg
Loaded 10985 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): 8491 out of 9314 total matches.
Matched with Tycho-2 9314 out of 17766 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
Forced-photometry filter: calibrated wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits -> calib.txt_param_ref_wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits (aperture=6.1)
Read 18110 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 111.8239 to 128.3329 deg, Dec +8.6240 to +19.2756 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 111.8239 to 128.3329 deg, Dec 8.6240 to 19.2756 deg
Loaded 10613 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): 8603 out of 9232 total matches.
Matched with Tycho-2 9232 out of 18110 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
Forced-photometry filter: calibrated wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits -> calib.txt_param_ref_wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits (aperture=6.4)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 5 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
2.0 pix Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
2.3 pix Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
3.2 pix fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
3.3 pix fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
Limiting magnitude estimates:
15.3 mag. Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
15.2 mag. Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
14.0 mag. fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
14.0 mag. fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 11.4 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
cp: cannot create regular file 'local_wcs_cache/': Not a directory
############ /tmp/tmp.mHeROAkPRl (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_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.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-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits' -> 'wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
WCS_IMAGE_NAME=wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
WCS-calibrated image found: wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
Checking if the catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat corresponding to the image wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits alredy exist and is non-empty...
Catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat corresponding to the image wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
WCS catalog name: wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1628, bad_region=0, passed=17766
Got 17766 stars (including 16092 good ones) from the SExtractor catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat
util/solve_plate_with_UCAC5 got 17766 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 4923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 4911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 17766 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.5 to 19.3)
Done reading UCAC5 zone files...
Matched 4923 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 17766 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 17766 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 4911 stars left (next iteration limit 5402)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits N_match=4911 sigma_overall_arcsec=0.388 sigma_q1_arcsec=0.502 sigma_q2_arcsec=0.356 sigma_q3_arcsec=0.359 sigma_q4_arcsec=0.337 n_q1=1418 n_q2=1183 n_q3=1248 n_q4=1062 worst_quadrant_to_overall_ratio=1.293
The image catalog is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits -region wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.7ykIFEkrxu (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.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-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits' -> 'wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
WCS_IMAGE_NAME=wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
WCS-calibrated image found: wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
Checking if the catalog wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits.wcscat corresponding to the image wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits alredy exist and is non-empty...
Catalog wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits.wcscat corresponding to the image wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
WCS catalog name: wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1405, bad_region=0, passed=18110
Got 18110 stars (including 16688 good ones) from the SExtractor catalog wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits.wcscat
util/solve_plate_with_UCAC5 got 18110 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 4910 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 18110 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 18110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 4909 matched stars entering correct_measured_positions(), 18110 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.41"
Excluding outliers - 4909 stars left (next iteration limit 5399)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits N_match=4909 sigma_overall_arcsec=0.426 sigma_q1_arcsec=0.325 sigma_q2_arcsec=0.506 sigma_q3_arcsec=0.394 sigma_q4_arcsec=0.487 n_q1=1013 n_q2=1330 n_q3=1115 n_q4=1451 worst_quadrant_to_overall_ratio=1.188
The image catalog is written to wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits -region wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.Gddba4zqmW (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_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.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_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
WCS-calibrated image found: wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
Checking if the catalog wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat corresponding to the image wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat corresponding to the image wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
WCS catalog name: wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=366, bad_region=0, passed=8273
Got 8273 stars (including 7898 good ones) from the SExtractor catalog wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat
util/solve_plate_with_UCAC5 got 8273 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.8'
Seting catalog search parameters based on the expected field of view 942.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013094 (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 0.010476 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 4887 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 8273 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 8273 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 8273 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4887 stars left (next iteration limit 5375)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4887 robust_rms=8.064 arcsec worst_quadrant_rms=15.668 arcsec
SIP_REFIT: SIP order 3 trial: matched=4887 robust_rms=0.391 arcsec worst_quadrant_rms=0.497 arcsec
SIP_REFIT: SIP order 5 trial: matched=4887 robust_rms=0.326 arcsec worst_quadrant_rms=0.405 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4887 robust_rms_before=0.996 arcsec robust_rms_before_corrected=0.330 arcsec robust_rms_after=0.326 arcsec worst_quadrant_rms_before=0.378 worst_quadrant_rms_after=0.405
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.378 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits N_match=4887 sigma_overall_arcsec=0.327 sigma_q1_arcsec=0.364 sigma_q2_arcsec=0.385 sigma_q3_arcsec=0.263 sigma_q4_arcsec=0.297 n_q1=1539 n_q2=985 n_q3=1433 n_q4=930 worst_quadrant_to_overall_ratio=1.178
The image catalog is written to wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits -region wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.GZ1MtmHB5w (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_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.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_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
WCS-calibrated image found: wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
Checking if the catalog wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits.wcscat corresponding to the image wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits.wcscat corresponding to the image wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
WCS catalog name: wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=381, bad_region=0, passed=8296
Got 8296 stars (including 7910 good ones) from the SExtractor catalog wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits.wcscat
util/solve_plate_with_UCAC5 got 8296 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 4888 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4887 matched stars entering correct_measured_positions(), 8296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4909 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 8296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 4888 matched stars entering correct_measured_positions(), 8296 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4888 stars left (next iteration limit 5375)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: SIP order 2 trial: matched=4888 robust_rms=8.028 arcsec worst_quadrant_rms=16.183 arcsec
SIP_REFIT: SIP order 3 trial: matched=4888 robust_rms=0.386 arcsec worst_quadrant_rms=0.429 arcsec
SIP_REFIT: SIP order 5 trial: matched=4888 robust_rms=0.326 arcsec worst_quadrant_rms=0.393 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4888 robust_rms_before=1.000 arcsec robust_rms_before_corrected=0.323 arcsec robust_rms_after=0.326 arcsec worst_quadrant_rms_before=0.372 worst_quadrant_rms_after=0.393
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.372 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits N_match=4888 sigma_overall_arcsec=0.322 sigma_q1_arcsec=0.359 sigma_q2_arcsec=0.380 sigma_q3_arcsec=0.254 sigma_q4_arcsec=0.310 n_q1=1534 n_q2=982 n_q3=1439 n_q4=933 worst_quadrant_to_overall_ratio=1.180
The image catalog is written to wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits -region wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
Saving the final (post-refit) wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits to local_wcs_cache/
'wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits' -> 'local_wcs_cache/wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits'
Saving the final (post-refit) wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits to local_wcs_cache/
'wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits' -> 'local_wcs_cache/wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits'
Saving the final (post-refit) wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits to local_wcs_cache/
'wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits' -> 'local_wcs_cache/wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits'
Saving the final (post-refit) wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits to local_wcs_cache/
'wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits' -> 'local_wcs_cache/wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits'
###################################
# Pre-local-correction WCS quality summary (see WCS_QUALITY_DIAG lines above)
ref1=Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits sigma_overall=0.388 worst_q_ratio=1.293
ref2=Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits sigma_overall=0.426 worst_q_ratio=1.188
new1=fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits sigma_overall=0.327 worst_q_ratio=1.178
new2=fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits sigma_overall=0.322 worst_q_ratio=1.180
reference average sigma_overall=0.407 worst_q_ratio=1.2405
warn-on-ratio threshold: 2.0x reference
###################################
Astrometric residual vector field (catalog-matched stars):
plot_astrometric_residuals_xy.py: wrote wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164_astrometric_residuals.png (4911 matched stars from wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.34 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152_astrometric_residuals.png (4909 matched stars from wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.38 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454_astrometric_residuals.png (4887 matched stars from wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
plot_astrometric_residuals_xy.py: wrote wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455_astrometric_residuals.png (4888 matched stars from wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits.wcscat.astrometric_residuals, image 9576x6388, median residual 0.29 arcsec)
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits'
Saving fully-calibrated image wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits'
Preparing the HTML report for the field Cnc-04-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits at 08:28:41.46 +13:28:27.1: 15.76 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits at 08:28:41.46 +13:28:27.1: 15.69 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out21840.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 6s
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 21812_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 21812_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:09:27.92 +14:39:51.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21840_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
Preparing report for the candidate 21840_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 00443_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 00443_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:16:30.66 +09:11:07.9 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05993_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 05993_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:34:00.59 +11:44:08.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05272_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 05272_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:16:33.63 +11:43:35.2 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 7s
Prepared the HTML report for the field Cnc-04-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 ####
08:28:41.46 +13:28:27.1
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --noflagimage --starmatchraius 5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
SExtractor catalog cache: saved Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.cat to cache
SExtractor catalog cache: saved Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.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-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
Creating symlink local_wcs_cache/wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
Creating symlink local_wcs_cache/wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
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-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits exists and is non-empty
wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits exists and is non-empty
wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits exists and is non-empty
wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits (1st reference image)
verification OK: wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
Image size: 941.7'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: 07:59:57.821 +13:59:32.16 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-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits (1st new image)
verification OK: wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
Image size: 942.8'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:59:55.719 +13:56:52.81 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:59:57.821 +13:59:32.16
Second-epoch image center 07:59:55.719 +13:56:52.81
Angular distance between the image centers 0.0451 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits (2nd new image)
verification OK: wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
Image size: 942.7'x626.8' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.91"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 07:59:58.694 +13:56:21.74 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:59:57.821 +13:59:32.16
Second-epoch image center 07:59:58.694 +13:56:21.74
Angular distance between the image centers 0.0530 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 07:59:55.719 +13:56:52.81
Second-epoch second image center 07:59:58.694 +13:56:21.74
Angular distance between the image centers 0.01481 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for a parallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits &> /tmp/tmp.29bMZlnVFt
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits &> /tmp/tmp.3YRorw4gwo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits &> /tmp/tmp.p3uK16fkZm
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits &> /tmp/tmp.dHQa6leSCe
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
Calibrating the magnitude scale
Found non-empty wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.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-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits and wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.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-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits and wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat
Found non-empty wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits and wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat
The reference image (wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits) and catalog (wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat) found
'wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat' -> 'wcsmag.cat'
Read 121795 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 111.5661 to 128.1518 deg, Dec +8.4481 to +19.3297 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 111.5661 to 128.1518 deg, Dec 8.4481 to 19.3297 deg
Loaded 11028 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): 7304 out of 9478 total matches.
Matched with Tycho-2 9478 out of 121795 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.779100
a=0.000000 b=1.000000 c=22.779100
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.49
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.49
Lightcurve magnitude calibration plot:
Preparing per-reference-image forced-photometry calibration (method=tycho2 band=V)
Read 121795 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 111.5661 to 128.1518 deg, Dec +8.4481 to +19.3297 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 111.5661 to 128.1518 deg, Dec 8.4481 to 19.3297 deg
Loaded 11028 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): 7304 out of 9478 total matches.
Matched with Tycho-2 9478 out of 121795 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00001.cat.aperture for wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
Forced-photometry filter: calibrated wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits -> calib.txt_param_ref_wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits (aperture=4.6)
Read 109990 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 111.8208 to 128.3356 deg, Dec +8.6056 to +19.2783 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 111.8208 to 128.3356 deg, Dec 8.6056 to 19.2783 deg
Loaded 10627 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): 7505 out of 9339 total matches.
Matched with Tycho-2 9339 out of 109990 detected stars.
util/calibrate_single_image_with_tycho2.sh: calibrated wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits via Tycho-2
Single-image forced-photometry magnitude calibration plot for wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits:
Forced-photometry filter: reusing the VaST-run aperture from image00002.cat.aperture for wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
Forced-photometry filter: calibrated wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits -> calib.txt_param_ref_wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits (aperture=4.9)
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 48 candidate transients before the final filtering. (Hard limit: 10000)
Median FWHM seeing for isolated stars:
1.8 pix Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
2.2 pix Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
3.1 pix fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
3.1 pix fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
Limiting magnitude estimates:
15.5 mag. Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
15.4 mag. Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
14.0 mag. fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
14.0 mag. fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.5 (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 15.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.29bMZlnVFt (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_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.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-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits' -> 'wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
WCS_IMAGE_NAME=wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
WCS-calibrated image found: wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
Checking if the catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat corresponding to the image wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits alredy exist and is non-empty...
Catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat corresponding to the image wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits
WCS catalog name: wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=11718, bad_region=4, passed=121750
Got 121750 stars (including 109791 good ones) from the SExtractor catalog wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat
util/solve_plate_with_UCAC5 got 121750 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.4 to 19.3)
Done reading UCAC5 zone files...
Matched 4919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 4912 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 121750 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 492 to 548 (Dec 8.4 to 19.3)
Done reading UCAC5 zone files...
Matched 4919 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 121750 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 4912 matched stars entering correct_measured_positions(), 121750 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 4912 stars left (next iteration limit 5403)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits N_match=4912 sigma_overall_arcsec=0.371 sigma_q1_arcsec=0.481 sigma_q2_arcsec=0.342 sigma_q3_arcsec=0.351 sigma_q4_arcsec=0.322 n_q1=1350 n_q2=1193 n_q3=1254 n_q4=1115 worst_quadrant_to_overall_ratio=1.296
The image catalog is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits -region wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.3YRorw4gwo (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.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-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits' -> 'wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits'
This WCS solution (astrometrynet) will be kept as is, not refit by util/solve_plate_with_UCAC5
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
WCS_IMAGE_NAME=wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
WCS-calibrated image found: wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
Checking if the catalog wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits.wcscat corresponding to the image wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits alredy exist and is non-empty...
Catalog wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits.wcscat corresponding to the image wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits
WCS catalog name: wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=39, blended=9995, bad_region=0, passed=109951
Got 109951 stars (including 99803 good ones) from the SExtractor catalog wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits.wcscat
util/solve_plate_with_UCAC5 got 109951 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.5'
Seting catalog search parameters based on the expected field of view 937.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013021 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010417 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 4911 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 109951 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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 493 to 548 (Dec 8.6 to 19.3)
Done reading UCAC5 zone files...
Matched 4921 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 109951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 4911 matched stars entering correct_measured_positions(), 109951 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 4911 stars left (next iteration limit 5402)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: util/identify.sh trusts the WCS of wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits (astrometrynet) - keeping it, no refit (set VAST_FORCE_SIP_REFIT=1 to refit anyway)
WCS_QUALITY_DIAG: file=Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits N_match=4911 sigma_overall_arcsec=0.423 sigma_q1_arcsec=0.307 sigma_q2_arcsec=0.491 sigma_q3_arcsec=0.393 sigma_q4_arcsec=0.490 n_q1=1038 n_q2=1366 n_q3=1075 n_q4=1432 worst_quadrant_to_overall_ratio=1.161
The image catalog is written to wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits -region wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.p3uK16fkZm (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_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.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_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
WCS-calibrated image found: wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
Checking if the catalog wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat corresponding to the image wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat corresponding to the image wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
WCS catalog name: wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=1961, bad_region=8, passed=43918
Got 43918 stars (including 41878 good ones) from the SExtractor catalog wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat
util/solve_plate_with_UCAC5 got 43918 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.8'
Seting catalog search parameters based on the expected field of view 942.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013094 (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 0.010476 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 4892 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4892 matched stars entering correct_measured_positions(), 43918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4906 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 43918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4893 matched stars entering correct_measured_positions(), 43918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 4893 stars left (next iteration limit 5381)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4893 robust_rms=7.942 arcsec worst_quadrant_rms=16.282 arcsec
SIP_REFIT: SIP order 3 trial: matched=4893 robust_rms=0.391 arcsec worst_quadrant_rms=0.480 arcsec
SIP_REFIT: SIP order 5 trial: matched=4893 robust_rms=0.327 arcsec worst_quadrant_rms=0.404 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4893 robust_rms_before=1.001 arcsec robust_rms_before_corrected=0.326 arcsec robust_rms_after=0.327 arcsec worst_quadrant_rms_before=0.371 worst_quadrant_rms_after=0.404
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.371 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits N_match=4893 sigma_overall_arcsec=0.317 sigma_q1_arcsec=0.348 sigma_q2_arcsec=0.373 sigma_q3_arcsec=0.258 sigma_q4_arcsec=0.298 n_q1=1528 n_q2=947 n_q3=1471 n_q4=947 worst_quadrant_to_overall_ratio=1.176
The image catalog is written to wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits -region wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
############ /tmp/tmp.dHQa6leSCe (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_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.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_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
WCS_IMAGE_NAME=wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
WCS-calibrated image found: wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
Checking if the catalog wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits.wcscat corresponding to the image wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits alredy exist and is non-empty...
Catalog wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits.wcscat corresponding to the image wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
WCS catalog name: wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits.wcscat
Excluding image region: 190.0 1039.0 192.0 1041.0 (defined in bad_region.lst)
Excluding image region: 226.0 1548.0 228.0 1550.0 (defined in bad_region.lst)
Excluding image region: 351.0 1875.0 353.0 1877.0 (defined in bad_region.lst)
Excluding image region: 501.0 5912.0 503.0 5914.0 (defined in bad_region.lst)
Excluding image region: 638.0 5545.0 640.0 5547.0 (defined in bad_region.lst)
Excluding image region: 724.0 2731.0 726.0 2733.0 (defined in bad_region.lst)
Excluding image region: 883.0 1376.0 885.0 1378.0 (defined in bad_region.lst)
Excluding image region: 901.0 3972.0 903.0 3974.0 (defined in bad_region.lst)
Excluding image region: 1151.0 918.0 1153.0 920.0 (defined in bad_region.lst)
Excluding image region: 1157.0 135.0 1159.0 137.0 (defined in bad_region.lst)
Excluding more image regions!.. (will not print them all)
Excluded a total of 50 image regions (defined in bad_region.lst).
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=14, blended=1997, bad_region=7, passed=44455
Got 44455 stars (including 42400 good ones) from the SExtractor catalog wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits.wcscat
util/solve_plate_with_UCAC5 got 44455 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 942.7'
Seting catalog search parameters based on the expected field of view 942.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013093 (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 0.010474 (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
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 4895 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 44455 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
UCAC5 local query limit 5000: matching up to 5000 detected stars, deepening the UCAC5 window to mag 15.50
Reading UCAC5 zone files...
Searching UCAC5 zones 490 to 549 (Dec 8.2 to 19.5)
Done reading UCAC5 zone files...
Matched 4908 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 44455 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Accuracy estimation diagnostic: 4894 matched stars entering correct_measured_positions(), 44455 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 4894 stars left (next iteration limit 5383)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
SIP_REFIT: wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits is a symbolic link - will not rewrite the WCS of whatever it points to, but will still refit the output catalog positions
SIP_REFIT: SIP order 2 trial: matched=4894 robust_rms=8.018 arcsec worst_quadrant_rms=16.608 arcsec
SIP_REFIT: SIP order 3 trial: matched=4894 robust_rms=0.390 arcsec worst_quadrant_rms=0.426 arcsec
SIP_REFIT: SIP order 5 trial: matched=4894 robust_rms=0.327 arcsec worst_quadrant_rms=0.396 arcsec
SIP_REFIT: selected SIP order 5
SIP_REFIT: order=5 matched=4894 robust_rms_before=0.999 arcsec robust_rms_before_corrected=0.322 arcsec robust_rms_after=0.327 arcsec worst_quadrant_rms_before=0.362 worst_quadrant_rms_after=0.396
SIP_REFIT: refit does not sufficiently improve on the solution it would replace (best worst-quadrant baseline 0.362 arcsec) - keeping the original
WCS_QUALITY_DIAG: file=fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits N_match=4894 sigma_overall_arcsec=0.320 sigma_q1_arcsec=0.357 sigma_q2_arcsec=0.370 sigma_q3_arcsec=0.256 sigma_q4_arcsec=0.305 n_q1=1532 n_q2=950 n_q3=1465 n_q4=947 worst_quadrant_to_overall_ratio=1.154
The image catalog is written to wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits.wcscat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits.wcscat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits -region wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits.wcscat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits.wcscat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
FORCED_PHOTOMETRY_CALIBRATION_METHOD=tycho2 - not using remote photometric catalogs, just stick with astrometry
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-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.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_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-44-15_20.00sec_-0.00C_LIGHTs_0454.fits
Saving fully-calibrated image wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.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_2026-09-07_CI_Cnc-04-Q1b1x1_054551_TTUQ1b1x1_1346127_qrlF6AVi/wcs_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455.fits
Preparing the HTML report for the field Cnc-04-Q1b1x1 with default.sex.telephoto_lens_vSTL
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits at 08:18:17.78 +15:41:38.1: 12.63 +/- 0.02 detection
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits at 07:35:15.19 +15:44:08.5: 13.28 +/- 0.03 detection
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits at 07:31:05.85 +11:13:20.3: 12.76 +/- 0.03 detection
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits at 07:35:15.19 +15:44:08.5: 13.31 +/- 0.03 detection
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits at 08:18:17.78 +15:41:38.1: 12.64 +/- 0.02 detection
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits at 07:31:05.85 +11:13:20.3: 12.79 +/- 0.03 detection
Forced photometry reference-image weighted average: 13.29 +/- 0.02
Forced photometry reference-image weighted average: 12.63 +/- 0.02
Forced photometry filter REJECTED candidate at 07:35:15.19 +15:44:08.5: ref_mag=13.29 +/- 0.02 new_mean_mag=13.1575 delta=0.13 (need > 0.90)
Forced photometry reference-image weighted average: 12.77 +/- 0.02
Forced photometry filter REJECTED candidate at 08:18:17.78 +15:41:38.1: ref_mag=12.63 +/- 0.02 new_mean_mag=12.4303 delta=0.20 (need > 0.90)
Forced photometry filter REJECTED candidate at 07:31:05.85 +11:13:20.3: ref_mag=12.77 +/- 0.02 new_mean_mag=12.6343 delta=0.14 (need > 0.90)
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits at 07:35:21.25 +17:23:28.0: 13.23 +/- 0.03 detection
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits at 08:17:09.06 +14:04:28.2: 15.88 +/- 0.30 detection
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits at 08:10:17.17 +09:11:18.1: 12.79 +/- 0.03 detection
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits at 07:35:21.25 +17:23:28.0: 13.21 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.22 +/- 0.02
Forced photometry filter REJECTED candidate at 07:35:21.25 +17:23:28.0: ref_mag=13.22 +/- 0.02 new_mean_mag=13.1636 delta=0.05 (need > 0.90)
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits at 08:17:09.06 +14:04:28.2: 15.17 +/- 0.17 detection
Forced photometry reference-image weighted average: 15.33 +/- 0.15
Forced photometry filter KEPT candidate at 08:17:09.06 +14:04:28.2: ref_mag=15.33 +/- 0.15 new_mean_mag=12.6812 delta=2.65 (need > 0.90)
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits at 07:36:02.46 +11:40:14.5: 15.99 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits at 08:07:16.83 +13:16:17.7: 13.21 +/- 0.03 detection
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits at 08:10:17.17 +09:11:18.1: 12.71 +/- 0.03 detection
Forced photometry reference-image weighted average: 12.75 +/- 0.02
Forced photometry filter REJECTED candidate at 08:10:17.17 +09:11:18.1: ref_mag=12.75 +/- 0.02 new_mean_mag=12.6818 delta=0.06 (need > 0.90)
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits at 07:46:38.78 +17:11:32.9: 16.07 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits at 07:36:02.46 +11:40:14.5: 15.87 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits at 08:07:16.83 +13:16:17.7: 13.28 +/- 0.04 detection
Forced photometry reference-image weighted average: 13.24 +/- 0.02
Forced photometry filter REJECTED candidate at 08:07:16.83 +13:16:17.7: ref_mag=13.24 +/- 0.02 new_mean_mag=13.0885 delta=0.15 (need > 0.90)
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits at 07:46:38.78 +17:11:32.9: 15.94 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-02-21_22-38-45_20.00sec_-14.90C_LIGHT_0164.fits at 07:44:10.10 +16:39:28.0: 16.15 +/- 99.00 upperlimit
Forced photometry on wcs_Cnc-04-Q1b1x1_2026-03-20_23-21-22_20.00sec_-15.00C_LIGHT_0152.fits at 07:44:10.10 +16:39:28.0: 16.04 +/- 99.00 upperlimit
Adding exclusion_list_local.txt__out105766.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out139400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out139618.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out139879.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 8s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 138697_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 138697_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 138698_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 138698_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:16:38.35 +16:23:42.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138699_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 138699_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:40:39.09 +18:49:41.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138701_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 138701_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:36:24.73 +12:53:43.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 138827_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 138827_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:28:41.46 +13:28:27.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 139064_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139064_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:46:21.16 +10:44:58.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 139128_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139128_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:40:47.57 +13:44:14.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 139136_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139136_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:29:07.35 +12:46:32.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139213_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139213_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 139219_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139219_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 139226_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139226_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:47:32.35 +09:39:33.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139230_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139230_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:37:56.92 +14:02:13.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139239_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139239_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:55:53.23 +10:26:53.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139241_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139241_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:04:46.77 +18:51:41.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 139343_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139343_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:06:54.11 +15:09:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139350_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139350_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:03:32.95 +12:09:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139365_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139365_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:49:08.08 +13:22:03.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 139400_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
Preparing report for the candidate 139400_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
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Considering the candidate 139429_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139429_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:01:23.60 +16:26:44.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 139442_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139442_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 139455_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139455_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:08:44.04 +16:44:22.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139464_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139464_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:47:34.22 +14:07:09.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139483_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139483_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:48:28.24 +18:20:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139486_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139486_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:29:25.04 +16:09:15.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139487_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139487_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 139498_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139498_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:31:41.12 +15:51:57.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139501_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139501_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:46:04.88 +16:26:43.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139513_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139513_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:35:08.00 +10:07:24.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139535_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139535_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:07:06.48 +15:07:25.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139542_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139542_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:09:58.56 +12:58:49.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139553_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139553_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:04:21.22 +12:16:11.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139564_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139564_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:24:10.43 +16:18:30.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139599_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139599_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
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Considering the candidate 139618_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
Preparing report for the candidate 139618_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
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Considering the candidate 139639_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139639_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:49:10.86 +18:02:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139675_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139675_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:01:22.51 +16:26:27.8 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 139714_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139714_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:52:00.49 +11:10:34.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 139879_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
Preparing report for the candidate 139879_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
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Considering the candidate 139880_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 139880_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:59:20.32 +13:50:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 01778_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 01778_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:16:30.66 +09:11:07.8 in the exclusion list exclusion_list_bbsc.txt ****
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Considering the candidate 72891_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 72891_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:30:57.16 +14:24:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 71131_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 71131_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:09:27.90 +14:39:51.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 16559_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 16559_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:13:38.13 +10:11:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39386_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 39386_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:34:00.58 +11:44:07.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 12407_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 12407_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 07:56:54.01 +09:42:37.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 105766_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
Preparing report for the candidate 105766_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
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Considering the candidate 33797_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 33797_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
**** FOUND 08:16:33.63 +11:43:35.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 45036_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455
The candidate 45036_fd_Cnc-04-Q1b1x1_2026-09-07_05-45-07_20.00sec_0.00C_LIGHTs_0455 did not pass the final checks
