This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 897080718081816960,2461138.7484,11.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 897080718081816960 20260408.2484 11.21CV 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
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J112.2176+36.8224,2461138.7484,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J112.2176+36.8224 20260408.2484 13.80CV 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
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461138.7484,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260408.2484 13.25CV 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
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461138.7484,14.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260408.2484 14.07CV 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
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GSC 02961-01723,2461138.7484,10.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GSC 02961-01723 20260408.2484 10.82CV 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
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J080119.41+345809.4,2461138.7484,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J080119.41+345809.4 20260408.2484 12.71CV 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
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
HM Aur,2461138.7484,8.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
HM Aur 20260408.2484 8.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSV 17407,2461138.7484,8.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSV 17407 20260408.2484 8.87CV 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
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASASSN-V J072346.02+410823.6,2461138.7484,10.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J072346.02+410823.6 20260408.2484 10.43CV 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
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 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VX Aur,2461138.7484,8.07,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VX Aur 20260408.2484 8.07CV 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: 2461083.71840488 12.02.2026 05:14:20.182 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
First image: 2461083.71840488 12.02.2026 05:14:20.182 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
Last image: 2461138.74867265 08.04.2026 05:57:55.317 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 15
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.48
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 10996
Objects passed selection criteria: 10984
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 9813.5
Average stars matched: 9584.25 (97.6639 %)
Memory usage VmPeak: 117548 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 01:04:37 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: 2461083.71840488 12.02.2026 05:14:20.182 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
First image: 2461083.71840488 12.02.2026 05:14:20.182 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
Last image: 2461138.74867265 08.04.2026 05:57:55.317 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 90
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.17
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: 24 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 70252
Objects passed selection criteria: 70077
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: 56547
Average stars matched: 54764.5 (96.8478 %)
Memory usage VmPeak: 175904 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Fri Apr 3 15:05:04 CDT 2026
VaST build number 1.0rc88-382-g85e3caff
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-03)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Apr 8 01:06:14 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/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
SExtractor catalog cache: saved Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat to cache
SExtractor catalog cache: saved Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.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: 2461138.74812042
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Re-using ../tns_transients_list.txt
'../tns_transients_list.txt' -> 'tns_transients_list.txt'
Plate-solving the images
wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits exists and is non-empty
Saving wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits to local_wcs_cache/
'wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits' -> 'local_wcs_cache/wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits'
wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits exists and is non-empty
Saving wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits to local_wcs_cache/
'wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits' -> 'local_wcs_cache/wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits'
wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits exists and is non-empty
Saving wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits to local_wcs_cache/
'wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits' -> 'local_wcs_cache/wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits'
wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits exists and is non-empty
Saving wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits to local_wcs_cache/
'wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits' -> 'local_wcs_cache/wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:38:11.466 +37:59:42.13
Second-epoch image center 07:38:10.857 +38:00:06.08
Angular distance between the image centers 0.0069 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:38:11.466 +37:59:42.13
Second-epoch image center 07:38:12.839 +38:00:19.14
Angular distance between the image centers 0.0112 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 07:38:10.857 +38:00:06.08
Second-epoch second image center 07:38:12.839 +38:00:19.14
Angular distance between the image centers 0.00745 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits &> /tmp/tmp.wx8U5tjqok
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits &> /tmp/tmp.sEbRBnENOL
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits &> /tmp/tmp.bwj0dCny5W
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits &> /tmp/tmp.9qrJVD3CUX
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits and wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits and wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
Found non-empty wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits and wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
The reference image (wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits) and catalog (wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat) found
'wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat' -> 'wcsmag.cat'
Read 16511 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 104.0628 to 125.3791 deg, Dec +32.1956 to +43.3101 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 104.0628 to 125.3791 deg, Dec 32.1956 to 43.3101 deg
Loaded 9690 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): 7062 out of 7673 total matches.
Matched with Tycho-2 7673 out of 16511 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.914913
a=0.000000 b=1.000000 c=22.914913
From vast_summary.log: estimated ref. image limiting mag.: -7.48
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.43
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.43
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 11 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
2.1 pix Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
3.8 pix fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
3.8 pix fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
Limiting magnitude estimates:
15.4 mag. Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
15.4 mag. Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
14.6 mag. fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
14.6 mag. fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
All-image limiting magnitude estimate: 14.6 (SNR ) 12.0 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.wx8U5tjqok (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.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_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits' -> 'wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
WCS-calibrated image found: wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
Checking if the catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
WCS catalog name: wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1352, passed=16511
Got 16511 stars (including 15129 good ones) from the SExtractor catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
util/solve_plate_with_UCAC5 got 16511 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 15975 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 958 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 15974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
WARNING: Accuracy estimation diagnostic: 958 matched stars entering correct_measured_positions(), 15974 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 958 stars left (next iteration limit 1053)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits -region wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.sEbRBnENOL (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.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_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits' -> 'wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
WCS-calibrated image found: wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
Checking if the catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
WCS catalog name: wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1382, passed=16387
Got 16387 stars (including 14973 good ones) from the SExtractor catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat
util/solve_plate_with_UCAC5 got 16387 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 15803 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 15805 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
WARNING: Accuracy estimation diagnostic: 956 matched stars entering correct_measured_positions(), 15805 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits -region wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.bwj0dCny5W (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_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.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_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
Checking if the catalog wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
WCS catalog name: wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1206, passed=10536
Got 10536 stars (including 9327 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits.cat
util/solve_plate_with_UCAC5 got 10536 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.86"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 10246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.92"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 10244 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.93"
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 10244 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 1.02"
Excluding outliers - 938 stars left (next iteration limit 1031)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits -region wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.9qrJVD3CUX (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_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
Checking if the catalog wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
WCS catalog name: wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1232, passed=10482
Got 10482 stars (including 9248 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 10482 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.84"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 937 matched stars entering correct_measured_positions(), 10141 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.4 to 43.3)
Done reading UCAC5 zone files...
Matched 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 10141 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.89"
WARNING: Accuracy estimation diagnostic: 938 matched stars entering correct_measured_positions(), 10141 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.99"
Excluding outliers - 938 stars left (next iteration limit 1030)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits -region wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits'
Saving fully-calibrated image wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits'
Saving fully-calibrated image wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits'
Saving fully-calibrated image wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits'
Preparing the HTML report for the field Lyn-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out12120.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 15s
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 20611_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 20611_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:56:57.69 +34:56:31.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20724_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 20724_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:52:34.54 +40:51:37.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20739_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 20739_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 08:06:02.34 +38:03:47.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 12120_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 12120_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09586_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 09586_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:39:26.41 +36:47:08.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08185_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 08185_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:25:33.79 +37:45:26.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 08343_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 08343_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:24:33.33 +37:35:38.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 05484_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 05484_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:23:34.86 +39:34:32.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 09545_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 09545_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:22:02.75 +36:45:39.9 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03751_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 03751_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:24:08.83 +40:40:17.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03442_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 03442_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:18:02.25 +40:53:00.6 in the exclusion list exclusion_list_bsc.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 17s
Prepared the HTML report for the field Lyn-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:21:20.22 +35:15:57.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
SExtractor catalog cache: saved Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat to cache
SExtractor catalog cache: saved Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
Creating symlink local_wcs_cache/wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits exists and is non-empty
wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits exists and is non-empty
wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits exists and is non-empty
wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:38:11.466 +37:59:42.13
Second-epoch image center 07:38:10.857 +38:00:06.08
Angular distance between the image centers 0.0069 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:38:11.466 +37:59:42.13
Second-epoch image center 07:38:12.839 +38:00:19.14
Angular distance between the image centers 0.0112 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 07:38:10.857 +38:00:06.08
Second-epoch second image center 07:38:12.839 +38:00:19.14
Angular distance between the image centers 0.00745 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits &> /tmp/tmp.TzT5XMtI3o
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits &> /tmp/tmp.Vm1IaA8gMA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits &> /tmp/tmp.4trY635UJp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits &> /tmp/tmp.TM9VkG0uzM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits and wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits and wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
Found non-empty wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits and wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
The reference image (wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits) and catalog (wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat) found
'wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat' -> 'wcsmag.cat'
Read 100593 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 104.0399 to 125.3938 deg, Dec +32.1488 to +43.3176 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 104.0399 to 125.3938 deg, Dec 32.1488 to 43.3176 deg
Loaded 9777 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): 6288 out of 7750 total matches.
Matched with Tycho-2 7750 out of 100593 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.795616
a=0.000000 b=1.000000 c=22.795616
From vast_summary.log: estimated ref. image limiting mag.: -7.17
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.63
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.63
Magnitude calibration plot:
____ 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: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
1.9 pix Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
3.6 pix fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
3.6 pix fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
Limiting magnitude estimates:
15.6 mag. Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
15.6 mag. Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
14.7 mag. fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
14.7 mag. fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
All-image limiting magnitude estimate: 14.7 (SNR ) 14.0 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.TzT5XMtI3o (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.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_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits' -> 'wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
WCS-calibrated image found: wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
Checking if the catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
WCS catalog name: wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=7850, passed=100565
Got 100565 stars (including 92523 good ones) from the SExtractor catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat
util/solve_plate_with_UCAC5 got 100565 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 934 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 98986 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.1 to 43.3)
Done reading UCAC5 zone files...
Matched 952 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 98984 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
WARNING: Accuracy estimation diagnostic: 952 matched stars entering correct_measured_positions(), 98983 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 952 stars left (next iteration limit 1047)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits -region wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.Vm1IaA8gMA (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.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_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits' -> 'wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
WCS-calibrated image found: wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
Checking if the catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
WCS catalog name: wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=35, blended=7890, passed=100818
Got 100818 stars (including 92732 good ones) from the SExtractor catalog wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat
util/solve_plate_with_UCAC5 got 100818 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.4'
Seting catalog search parameters based on the expected field of view 941.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013075 (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 0.010460 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 935 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 99249 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.2 to 43.3)
Done reading UCAC5 zone files...
Matched 950 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 99246 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
WARNING: Accuracy estimation diagnostic: 950 matched stars entering correct_measured_positions(), 99245 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Excluding outliers - 950 stars left (next iteration limit 1045)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits -region wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.4trY635UJp (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_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.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_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
Checking if the catalog wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
WCS catalog name: wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=11, blended=6945, passed=46425
Got 46425 stars (including 39458 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits.cat
util/solve_plate_with_UCAC5 got 46425 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.80"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 45208 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 938 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 45208 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
WARNING: Accuracy estimation diagnostic: 936 matched stars entering correct_measured_positions(), 45208 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.90"
Excluding outliers - 936 stars left (next iteration limit 1029)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits -region wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.TM9VkG0uzM (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_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
Checking if the catalog wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
WCS catalog name: wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=16, blended=6985, passed=46632
Got 46632 stars (including 39612 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits.cat
util/solve_plate_with_UCAC5 got 46632 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 916 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.78"
Removing outliers...
Correcting the measured astrometric positions...
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 45532 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.3)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 45530 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.77"
WARNING: Accuracy estimation diagnostic: 935 matched stars entering correct_measured_positions(), 45530 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.88"
Excluding outliers - 935 stars left (next iteration limit 1028)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits -region wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.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_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/wcs_Lyn-05-Q2b1x1_2026-02-11_23-14-20_20.00sec_-14.90C_LIGHT_0203.fits
Saving fully-calibrated image wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/wcs_Lyn-05-Q2b1x1_2026-02-11_23-15-15_20.00sec_-15.00C_LIGHT_0204.fits
Saving fully-calibrated image wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.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_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-07_20.00sec_-4.90C_LIGHT_0061.fits
Saving fully-calibrated image wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-04-08_CI_Lyn-05-Q2b1x1_005940_TTUQ2b1x1_29964_RCSAkLEH/wcs_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062.fits
Preparing the HTML report for the field Lyn-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out116581.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116583.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116584.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116590.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116592.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116593.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116594.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116603.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116608.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out117182.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out116580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out116612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out117268.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out17494.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out18042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out25756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out35451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out79575.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 16s
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: 5s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116573_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 116573_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116580_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 116580_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116581_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 116581_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:15:20.56 +41:51:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 1.671 949357719978591872 108.83622032103 +41.86251858149 13.3188 12.8407 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.671#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116583_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 116583_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:20:41.47 +35:41:34.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116584_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 116584_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:46:46.45 +34:53:08.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116590_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 116590_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:33:27.23 +38:42:54.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116592_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 116592_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:21:24.00 +39:04:21.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116593_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 116593_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:57:46.73 +35:41:20.2 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.91, MAG_FAINT_SEARCH_LIMIT=14.89)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116594_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 116594_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:31:38.76 +37:58:11.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116603_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 116603_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:18:31.49 +35:02:21.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 2.271 896745504474423296 109.63180883349 +35.03981173291 13.1167 12.6601 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116608_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 116608_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:20:36.18 +35:59:08.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116612_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 116612_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116849_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 116849_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 08:07:53.16 +38:35:52.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116875_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 116875_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:42:50.63 +34:00:35.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116947_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 116947_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 08:06:10.89 +34:40:32.8 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 116963_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 116963_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:38:12.10 +38:17:13.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117005_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 117005_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 08:03:35.43 +36:22:52.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117092_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 117092_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 08:01:35.64 +34:39:21.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117174_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 117174_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:44:35.09 +35:50:34.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117182_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 117182_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:33:31.72 +37:10:20.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 5.695 898665286135806720 113.38398753881 +37.17159165420 13.6972 13.2274 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117199_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 117199_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:57:02.86 +36:19:36.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 117268_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 117268_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25756_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 25756_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51921_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 51921_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:24:33.34 +37:35:38.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 79575_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 79575_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32582_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 32582_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:23:34.83 +39:34:32.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 74645_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 74645_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (26.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 89648_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 89648_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:21:20.23 +35:15:57.6 in the exclusion list exclusion_list_local.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11258_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 11258_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (27.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 51065_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 51065_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:25:33.77 +37:45:27.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21537_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 21537_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35451_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 35451_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 18042_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 18042_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 73370_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 73370_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:39:26.42 +36:47:08.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 17494_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
Preparing report for the candidate 17494_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 35861_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 35861_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
Rejecting candidate due to large distance (27.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14448_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 14448_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 08:05:01.80 +41:11:20.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 42895_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 42895_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:40:14.46 +38:20:40.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 55647_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 55647_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:33:24.91 +37:11:16.6 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 49544_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 49544_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:46:39.00 +37:31:05.5 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27348_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 27348_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:37:17.74 +40:01:28.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 37877_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 37877_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:22:13.35 +38:59:41.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 87988_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 87988_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:38:32.92 +35:03:01.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 84133_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 84133_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:39:09.79 +34:35:07.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72574_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 72574_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:22:02.72 +36:45:39.8 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 38959_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 38959_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:17:42.48 +38:52:32.0 in the exclusion list exclusion_list_tycho2.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21550_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 21550_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
**** FOUND 07:24:08.78 +40:40:17.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 19675_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062
The candidate 19675_fd_Lyn-05-Q2b1x1_2026-04-08_00-57-55_20.00sec_-4.90C_LIGHT_0062 did not pass the final checks
