This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I
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!
TCP 2026 04 13.2819* 08 46 07.77 +48 58 22.4 13.6 U UMa 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461143.7819,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260413.2819 13.56CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J120.8997+55.4182,2461143.7819,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J120.8997+55.4182 20260413.2819 13.37CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1032115864256342272,2461143.7819,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1032115864256342272 20260413.2819 12.94CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461143.7819,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260413.2819 13.37CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461143.7819,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260413.2819 13.69CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J119.8112+58.2812,2461143.7819,14.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J119.8112+58.2812 20260413.2819 14.11CV 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 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J126.1119+54.0652,2461143.7819,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J126.1119+54.0652 20260413.2819 14.21CV 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
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461058.81301528 18.01.2026 07:30:34.520 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
First image: 2461058.81301528 18.01.2026 07:30:34.520 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Last image: 2461143.78229221 13.04.2026 06:46:20.047 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
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: 3 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): 10173
Objects passed selection criteria: 10152
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: 9066.75
Average stars matched: 8924.75 (98.4338 %)
Memory usage VmPeak: 115640 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 01:48:12 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: 2461058.81301528 18.01.2026 07:30:34.520 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
First image: 2461058.81301528 18.01.2026 07:30:34.520 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Last image: 2461143.78229221 13.04.2026 06:46:20.047 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 50
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.20
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: 18 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): 57384
Objects passed selection criteria: 57244
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: 52986.8
Average stars matched: 51659.2 (97.4947 %)
Memory usage VmPeak: 157020 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Sun Apr 12 15:05:06 CDT 2026
VaST build number 1.0rc89-12-g393f88de
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-12)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Mon Apr 13 01:55:51 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
SExtractor catalog cache: saved Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat to cache
SExtractor catalog cache: saved Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.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: 2461143.78157824
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-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits exists and is non-empty
Saving wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits to local_wcs_cache/
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits exists and is non-empty
Saving wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits to local_wcs_cache/
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits exists and is non-empty
Saving wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits to local_wcs_cache/
'wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits' -> 'local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits'
wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits exists and is non-empty
Saving wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits to local_wcs_cache/
'wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits' -> 'local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits'
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:28:35.075 +53:59:05.09
Second-epoch image center 08:28:25.025 +54:04:01.50
Angular distance between the image centers 0.0859 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 08:28:35.075 +53:59:05.09
Second-epoch image center 08:28:25.971 +54:03:19.90
Angular distance between the image centers 0.0742 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 08:28:25.025 +54:04:01.50
Second-epoch second image center 08:28:25.971 +54:03:19.90
Angular distance between the image centers 0.01179 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-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits &> /tmp/tmp.w8Rv9qchDO
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits &> /tmp/tmp.gJBp6SCUl0
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits &> /tmp/tmp.ww0B5c8n3e
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits &> /tmp/tmp.OJEs3ra924
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
Found non-empty wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
The reference image (wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits) and catalog (wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat) found
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat' -> 'wcsmag.cat'
Read 10732 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 113.1029 to 142.4921 deg, Dec +47.7241 to +59.2635 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 113.1029 to 142.4921 deg, Dec 47.7241 to 59.2635 deg
Loaded 7241 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): 20 out of 20 total matches.
Matched with Tycho-2 20 out of 10732 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.854505
a=0.000000 b=1.000000 c=22.854505
From vast_summary.log: estimated ref. image limiting mag.: -7.42
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 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
2.1 pix Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
2.2 pix fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
2.2 pix fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
Limiting magnitude estimates:
15.4 mag. Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
15.4 mag. Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
14.9 mag. fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
14.9 mag. fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
All-image limiting magnitude estimate: 14.9 (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.w8Rv9qchDO (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> 'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS-calibrated image found: wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Checking if the catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS catalog name: wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=751, passed=10732
Got 10732 stars (including 9968 good ones) from the SExtractor catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
util/solve_plate_with_UCAC5 got 10732 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.4'
Seting catalog search parameters based on the expected field of view 927.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012881 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010304 (37.1 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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 178 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 147 matched stars entering correct_measured_positions(), 124 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.17"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 141 matched stars entering correct_measured_positions(), 1637 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.63"
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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 223 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 205 matched stars entering correct_measured_positions(), 1671 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.34"
Accuracy estimation diagnostic: 202 matched stars entering correct_measured_positions(), 2144 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.08"
Excluding outliers - 202 stars left (next iteration limit 155)
The image catalog is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits -region wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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.gJBp6SCUl0 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> 'wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS-calibrated image found: wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Checking if the catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS catalog name: wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=785, passed=10668
Got 10668 stars (including 9872 good ones) from the SExtractor catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
util/solve_plate_with_UCAC5 got 10668 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.5'
Seting catalog search parameters based on the expected field of view 927.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012882 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010306 (37.1 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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 172 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 142 matched stars entering correct_measured_positions(), 117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 11.19"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 137 matched stars entering correct_measured_positions(), 1584 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.80"
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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 219 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 199 matched stars entering correct_measured_positions(), 1618 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.56"
Accuracy estimation diagnostic: 198 matched stars entering correct_measured_positions(), 2106 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.06"
Excluding outliers - 198 stars left (next iteration limit 150)
The image catalog is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits -region wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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.ww0B5c8n3e (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_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.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_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=448, passed=7560
Got 7560 stars (including 7105 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits.cat
util/solve_plate_with_UCAC5 got 7560 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 749 (Dec 47.9 to 59.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 965 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 7439 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 689 to 749 (Dec 47.9 to 59.4)
Done reading UCAC5 zone files...
Matched 975 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 7440 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 975 matched stars entering correct_measured_positions(), 7440 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 975 stars left (next iteration limit 1072)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.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.OJEs3ra924 (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_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.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_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=454, passed=7531
Got 7531 stars (including 7071 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits.cat
util/solve_plate_with_UCAC5 got 7531 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 689 to 749 (Dec 47.8 to 59.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 967 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.30"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 7408 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 689 to 749 (Dec 47.8 to 59.4)
Done reading UCAC5 zone files...
Matched 976 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 7410 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Accuracy estimation diagnostic: 976 matched stars entering correct_measured_positions(), 7410 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 976 stars left (next iteration limit 1073)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.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-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
Saving fully-calibrated image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
Saving fully-calibrated image wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits'
Saving fully-calibrated image wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits'
Preparing the HTML report for the field Lyn-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20557.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 1s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20507_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 20507_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:40:49.50 +50:08:12.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20557_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 20557_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:28:18.74 +55:46:33.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02150_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 02150_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 07:55:51.06 +57:11:51.3 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Lyn-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
SExtractor catalog cache: saved Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat to cache
SExtractor catalog cache: saved Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Creating symlink local_wcs_cache/wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.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-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits exists and is non-empty
wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits exists and is non-empty
wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits exists and is non-empty
wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits exists and is non-empty
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:28:35.075 +53:59:05.09
Second-epoch image center 08:28:25.025 +54:04:01.50
Angular distance between the image centers 0.0859 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 08:28:35.075 +53:59:05.09
Second-epoch image center 08:28:25.971 +54:03:19.90
Angular distance between the image centers 0.0742 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 08:28:25.025 +54:04:01.50
Second-epoch second image center 08:28:25.971 +54:03:19.90
Angular distance between the image centers 0.01179 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-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits &> /tmp/tmp.JaUyXqJEjU
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits &> /tmp/tmp.lRaaqyFDb4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits &> /tmp/tmp.PYvDaa5Aq1
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits &> /tmp/tmp.5NEnYMoAMs
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
Found non-empty wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits and wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
The reference image (wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits) and catalog (wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat) found
'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat' -> 'wcsmag.cat'
Read 60990 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 113.0237 to 142.6172 deg, Dec +47.6792 to +59.2703 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 113.0237 to 142.6172 deg, Dec 47.6792 to 59.2703 deg
Loaded 7317 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): 20 out of 25 total matches.
Matched with Tycho-2 25 out of 60990 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.056610
a=0.000000 b=1.000000 c=22.056610
From vast_summary.log: estimated ref. image limiting mag.: -7.20
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.86
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.86
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 41 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
2.0 pix Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
2.1 pix fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
2.1 pix fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
Limiting magnitude estimates:
14.9 mag. Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
14.9 mag. Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
14.3 mag. fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
14.3 mag. fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
All-image limiting magnitude estimate: 14.3 (SNR ) 13.7 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.JaUyXqJEjU (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> 'wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS-calibrated image found: wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Checking if the catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS catalog name: wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=3457, passed=60971
Got 60971 stars (including 57409 good ones) from the SExtractor catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
util/solve_plate_with_UCAC5 got 60971 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.4'
Seting catalog search parameters based on the expected field of view 927.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012881 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010304 (37.1 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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 172 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 142 matched stars entering correct_measured_positions(), 118 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.89"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 135 matched stars entering correct_measured_positions(), 9052 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.46"
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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 218 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 192 matched stars entering correct_measured_positions(), 9088 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.40"
Accuracy estimation diagnostic: 189 matched stars entering correct_measured_positions(), 12156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 6.55"
Excluding outliers - 189 stars left (next iteration limit 148)
The image catalog is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits -region wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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.lRaaqyFDb4 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> 'wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS-calibrated image found: wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Checking if the catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS catalog name: wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=3501, passed=61060
Got 61060 stars (including 57445 good ones) from the SExtractor catalog wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
util/solve_plate_with_UCAC5 got 61060 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.5'
Seting catalog search parameters based on the expected field of view 927.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012882 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010306 (37.1 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 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 172 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 140 matched stars entering correct_measured_positions(), 117 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 10.18"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 133 matched stars entering correct_measured_positions(), 8718 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.40"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 748 (Dec 47.7 to 59.3)
Done reading UCAC5 zone files...
Matched 219 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 189 matched stars entering correct_measured_positions(), 8757 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 9.37"
Accuracy estimation diagnostic: 188 matched stars entering correct_measured_positions(), 12273 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 7.11"
Excluding outliers - 188 stars left (next iteration limit 146)
The image catalog is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits -region wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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.PYvDaa5Aq1 (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_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.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_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=2035, passed=45727
Got 45727 stars (including 43621 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits.cat
util/solve_plate_with_UCAC5 got 45727 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 749 (Dec 47.8 to 59.4)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 963 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 45155 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 749 (Dec 47.8 to 59.4)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 45156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 45156 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.28"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.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.5NEnYMoAMs (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_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.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_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=2047, passed=45699
Got 45699 stars (including 43566 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits.cat
util/solve_plate_with_UCAC5 got 45699 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.7'
Seting catalog search parameters based on the expected field of view 941.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013079 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010463 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 688 to 749 (Dec 47.8 to 59.4)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 964 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 45099 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
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 688 to 749 (Dec 47.8 to 59.4)
Done reading UCAC5 zone files...
Matched 974 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 45099 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.29"
Accuracy estimation diagnostic: 974 matched stars entering correct_measured_positions(), 45099 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.27"
Excluding outliers - 974 stars left (next iteration limit 1071)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.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-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/wcs_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Saving fully-calibrated image wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/wcs_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Saving fully-calibrated image wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.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_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-45-18_20.00sec_-4.90C_LIGHTs_0090.fits
Saving fully-calibrated image wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.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_2026-04-13_CI_Lyn-02-Q1b1x1_014714_TTUQ1b1x1_12141_Lojmcy3I/wcs_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091.fits
Preparing the HTML report for the field Lyn-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out75390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75398.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75402.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75404.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75678.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75742.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75873.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75894.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75909.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out75951.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out75389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75396.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75603.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75711.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75878.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out75915.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 4s
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Considering the candidate 75389_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
Preparing report for the candidate 75389_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
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Considering the candidate 75390_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75390_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 07:43:34.00 +53:41:02.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 0.850 984554942609313408 115.89127042013 +53.68405856722 14.7498 14.4294 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75393_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75393_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 07:46:52.41 +54:12:25.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 0.529 984959013132701696 116.71859396312 +54.20718341433 14.0879 13.6386 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.529#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75396_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
Preparing report for the candidate 75396_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
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Considering the candidate 75398_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75398_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 09:01:40.28 +49:19:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.16, MAG_FAINT_SEARCH_LIMIT=14.14)GAIADR2_OUTPUT=# 1.175 1015772826500984832 135.41737017191 +49.32404098554 13.8087 13.3054 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75402_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75402_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:02:11.04 +56:03:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 0.271 1081072031800560640 120.54613465766 +56.06354954824 14.0818 13.6027 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.271#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75403_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75403_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:33:53.11 +56:23:55.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75404_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75404_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:02:16.27 +56:45:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.97, MAG_FAINT_SEARCH_LIMIT=13.95)GAIADR2_OUTPUT=# 1.771 1081525923944381568 120.56764846168 +56.76401423770 13.8465 13.3308 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.771#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75405_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75405_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 07:51:43.97 +49:23:05.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75407_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75407_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:11:25.34 +56:03:00.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 1.141 1033359240109292032 122.85570521086 +56.05033738226 13.5015 12.8806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.141#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75416_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75416_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 07:40:38.56 +49:30:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75464_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75464_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:02:15.70 +51:17:43.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75493_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75493_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:09:34.25 +55:10:07.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75498_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75498_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:08:37.65 +51:32:04.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75514_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75514_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 07:45:03.02 +55:43:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75527_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75527_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:01:18.99 +54:26:37.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75539_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75539_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 09:05:24.27 +48:33:39.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 75562_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75562_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 07:41:03.29 +57:04:57.6 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 75571_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75571_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 07:45:34.70 +56:36:46.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75603_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
Preparing report for the candidate 75603_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
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Considering the candidate 75660_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75660_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 07:48:59.37 +56:45:56.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75667_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75667_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:39:51.58 +56:11:22.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75678_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75678_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 07:46:56.62 +55:21:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 0.445 985873257051285504 116.73612987959 +55.36433058378 14.2558 13.7618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75688_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75688_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:11:50.70 +49:33:55.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75693_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75693_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 07:48:48.97 +55:26:43.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75706_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75706_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:28:05.07 +58:44:43.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75707_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75707_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 07:59:02.52 +58:53:40.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75711_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
Preparing report for the candidate 75711_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
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Considering the candidate 75742_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75742_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 07:41:31.12 +51:18:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.41, MAG_FAINT_SEARCH_LIMIT=14.39)GAIADR2_OUTPUT=# 2.089 982686082079275648 115.38043895988 +51.30284487448 14.1652 13.7095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75753_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75753_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:30:19.07 +54:28:48.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75764_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75764_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 07:54:19.47 +52:58:54.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75803_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
Preparing report for the candidate 75803_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
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Considering the candidate 75808_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75808_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:01:37.86 +55:27:59.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 75873_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75873_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:31:14.87 +58:56:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 0.917 1035462262256190336 127.81170600604 +58.93889223486 14.8226 14.1346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.917#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75878_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
Preparing report for the candidate 75878_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
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Considering the candidate 75894_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75894_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:23:56.90 +57:26:54.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.074 1034902473398176640 125.98673014167 +57.44826993436 14.7988 14.1142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.074#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75909_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75909_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:09:30.14 +58:48:19.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)GAIADR2_OUTPUT=# 1.056 1083345581328158208 122.37514502109 +58.80551894774 15.0365 14.4962 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 75915_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
Preparing report for the candidate 75915_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
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Considering the candidate 75951_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 75951_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:08:43.23 +55:33:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 0.922 1033319073575233536 122.17970788079 +55.55823353397 15.0676 14.4634 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.922#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 48804_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 48804_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks
**** FOUND 08:40:49.49 +50:08:12.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 11108_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091
The candidate 11108_fd_Lyn-02-Q1b1x1_2026-04-13_01-46-20_20.00sec_-4.90C_LIGHTs_0091 did not pass the final checks