This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc90 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461149.6531,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1531 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
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
ZTF J061829.30+382101.1,2461149.6531,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J061829.30+382101.1 20260419.1531 13.67CV 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,2461149.6531,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1531 13.41CV 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
VARIABLE_NAME,2461149.6531,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260419.1531 13.60CV 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,2461149.6531,14.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260419.1531 14.88CV 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
ASASSN-V J062800.27+394011.8,2461149.6531,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J062800.27+394011.8 20260419.1531 13.46CV 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: 2461061.71871545 21.01.2026 05:14:47.015 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461061.71871545 21.01.2026 05:14:47.015 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461149.65345631 19.04.2026 03:40:48.625 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 15
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.64
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: 7 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): 20917
Objects passed selection criteria: 20816
Measurements per detected object (mean, median, min, max): 2.9 2.0 2 4
Measurements per selected object (mean, median, min, max): 3.0 2.0 2 4
Average stars detected per image: 16027.2
Average stars matched: 14666 (91.5067 %)
Memory usage VmPeak: 122832 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Apr 18 22:44:31 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: 2461061.71871545 21.01.2026 05:14:47.015 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
First image: 2461061.71871545 21.01.2026 05:14:47.015 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Last image: 2461149.65345631 19.04.2026 03:40:48.625 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 104
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.30
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: 75 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): 145835
Objects passed selection criteria: 145414
Measurements per detected object (mean, median, min, max): 2.8 2.0 2 4
Measurements per selected object (mean, median, min, max): 2.8 2.0 2 4
Average stars detected per image: 108749
Average stars matched: 99500 (91.4949 %)
Memory usage VmPeak: 1961736 kB
Software: VaST 1.0rc90 compiled with gcc (Gentoo 15.2.1_p20260214 p5) 15.2.1 20260214
VaST compiled on Thu Apr 16 15:05:05 CDT 2026
VaST build number 1.0rc89-19-g55e4b97d
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-04-16)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Apr 18 22:48:16 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
SExtractor catalog cache: saved Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.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: 2461149.65279584
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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
Saving wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits to local_wcs_cache/
'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits' -> 'local_wcs_cache/wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits'
wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits exists and is non-empty
Saving wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits to local_wcs_cache/
'wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits' -> 'local_wcs_cache/wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits'
wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits exists and is non-empty
Saving wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits to local_wcs_cache/
'wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits' -> 'local_wcs_cache/wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits'
wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits exists and is non-empty
Saving wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits to local_wcs_cache/
'wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits' -> 'local_wcs_cache/wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits'
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits (1st reference image)
verification OK: wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:32:43.667 +37:59:56.47 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits (1st new image)
verification OK: wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
Image size: 937.1'x623.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:33:10.834 +37:58:13.41 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:32:43.667 +37:59:56.47
Second-epoch image center 06:33:10.834 +37:58:13.41
Angular distance between the image centers 0.0937 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits (2nd new image)
verification OK: wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
Image size: 937.1'x623.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:33:14.023 +37:57:48.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:32:43.667 +37:59:56.47
Second-epoch image center 06:33:14.023 +37:57:48.60
Angular distance between the image centers 0.1058 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 06:33:10.834 +37:58:13.41
Second-epoch second image center 06:33:14.023 +37:57:48.60
Angular distance between the image centers 0.01254 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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.Q03xmwisLA
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits &> /tmp/tmp.RCR2YxFQzz
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits &> /tmp/tmp.TGQfwGfksM
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits &> /tmp/tmp.MCt7EnSWQ9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat' -> 'wcsmag.cat'
Read 22646 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.2031 to 108.5019 deg, Dec +32.0173 to +43.3852 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 87.2031 to 108.5019 deg, Dec 32.0173 to 43.3852 deg
Loaded 14726 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): 10210 out of 11206 total matches.
Matched with Tycho-2 11206 out of 22646 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.938798
a=0.000000 b=1.000000 c=22.938798
From vast_summary.log: estimated ref. image limiting mag.: -7.64
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.30
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.30
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 12 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
2.0 pix Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
2.0 pix Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
2.8 pix fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
2.8 pix fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
Limiting magnitude estimates:
15.3 mag. Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
15.3 mag. Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
14.8 mag. fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
14.8 mag. fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
All-image limiting magnitude estimate: 14.8 (SNR ) 12.1 (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.Q03xmwisLA (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2024, passed=22646
Got 22646 stars (including 20590 good ones) from the SExtractor catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 22646 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 923 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 21795 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 934 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 21794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.32"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 21794 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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.RCR2YxFQzz (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits' -> 'wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS-calibrated image found: wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Checking if the catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS catalog name: wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=2057, passed=22538
Got 22538 stars (including 20456 good ones) from the SExtractor catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat
util/solve_plate_with_UCAC5 got 22538 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 918 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 21822 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 610 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 937 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 21823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Accuracy estimation diagnostic: 934 matched stars entering correct_measured_positions(), 21823 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 934 stars left (next iteration limit 1027)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits -region wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.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.TGQfwGfksM (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_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.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_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
Checking if the catalog wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
WCS catalog name: wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1616, passed=17675
Got 17675 stars (including 16051 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits.cat
util/solve_plate_with_UCAC5 got 17675 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 908 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 17329 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 926 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 17330 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Accuracy estimation diagnostic: 923 matched stars entering correct_measured_positions(), 17330 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 923 stars left (next iteration limit 1015)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits -region wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.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.MCt7EnSWQ9 (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_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.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_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
Checking if the catalog wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
WCS catalog name: wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1648, passed=17605
Got 17605 stars (including 15950 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits.cat
util/solve_plate_with_UCAC5 got 17605 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 17203 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 927 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 17204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Accuracy estimation diagnostic: 924 matched stars entering correct_measured_positions(), 17204 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 924 stars left (next iteration limit 1016)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits -region wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits'
Saving fully-calibrated image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits'
Saving fully-calibrated image wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits'
Saving fully-calibrated image wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits'
Preparing the HTML report for the field Aur-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out34802.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 32387_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 32387_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:28:01.81 +36:05:00.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 32996_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 32996_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:52:42.33 +33:55:50.5 in the exclusion list exclusion_list_bbsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 33192_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 33192_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:50:52.89 +37:33:10.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34036_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 34036_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:36:16.56 +41:49:34.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34358_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 34358_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:33:14.39 +34:30:38.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34413_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 34413_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:29:04.97 +37:45:49.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34427_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 34427_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:38:15.64 +35:21:56.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34460_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 34460_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:40:32.79 +40:17:06.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34479_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 34479_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:40:37.15 +37:03:06.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34482_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 34482_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:27:43.29 +34:51:25.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34555_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 34555_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:34:06.84 +34:03:27.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 34802_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 34802_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:25:14.00 +36:26:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.984 954810090766302720 096.30852828410 +36.43477616922 11.8173 10.8417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.984#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 2s
Prepared the HTML report for the field Aur-04-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
SExtractor catalog cache: saved Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat to cache
SExtractor catalog cache: saved Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Creating symlink local_wcs_cache/wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
Creating symlink local_wcs_cache/wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits exists and is non-empty
wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits exists and is non-empty
wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits exists and is non-empty
wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits exists and is non-empty
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits (1st reference image)
verification OK: wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Image size: 941.5'x627.0' 15.7(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.90"/pix along the X axis and 5.89"/pix along the Y axis
Image center: 06:32:43.667 +37:59:56.47 J2000 4789.000 3195.000
###################################
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits (1st new image)
verification OK: wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
Image size: 937.1'x623.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:33:10.834 +37:58:13.41 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 06:32:43.667 +37:59:56.47
Second-epoch image center 06:33:10.834 +37:58:13.41
Angular distance between the image centers 0.0937 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# fov_of_wcs_calibrated_image.sh output for wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits (2nd new image)
verification OK: wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
Image size: 937.1'x623.9' 15.6(deg)x10.4(deg) 9576x6388 pix
Image scale: 5.87"/pix along the X axis and 5.86"/pix along the Y axis
Image center: 06:33:14.023 +37:57:48.60 J2000 4789.000 3195.000
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 06:32:43.667 +37:59:56.47
Second-epoch image center 06:33:14.023 +37:57:48.60
Angular distance between the image centers 0.1058 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 06:33:10.834 +37:58:13.41
Second-epoch second image center 06:33:14.023 +37:57:48.60
Angular distance between the image centers 0.01254 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/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits &> /tmp/tmp.FmZHXHLZPo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits &> /tmp/tmp.T9PoaS06IK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits &> /tmp/tmp.0YxcosGoU4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits &> /tmp/tmp.TJ6kPPRQFq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
Calibrating the magnitude scale
Found non-empty wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
Found non-empty wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits and wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
The reference image (wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits) and catalog (wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat) found
'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat' -> 'wcsmag.cat'
Read 160824 stars from the SExtractor catalog wcsmag.cat
Detected star coordinate range: RA 87.1754 to 108.5197 deg, Dec +31.9766 to +43.3901 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 87.1754 to 108.5197 deg, Dec 31.9766 to 43.3901 deg
Loaded 14824 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): 8279 out of 11458 total matches.
Matched with Tycho-2 11458 out of 160824 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.781706
a=0.000000 b=1.000000 c=22.781706
From vast_summary.log: estimated ref. image limiting mag.: -7.30
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.48
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.48
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 88 candidate transients before the final filtering. (Hard limit: 8000)
Median FWHM seeing for isolated stars:
1.9 pix Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
1.9 pix Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
2.7 pix fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
2.7 pix fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
Limiting magnitude estimates:
15.5 mag. Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
15.5 mag. Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
14.9 mag. fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
14.9 mag. fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
All-image limiting magnitude estimate: 14.9 (SNR ) 14.3 (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.FmZHXHLZPo (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits' -> 'wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS-calibrated image found: wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Checking if the catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
WCS catalog name: wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=32, blended=18360, passed=160792
Got 160792 stars (including 142160 good ones) from the SExtractor catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat
util/solve_plate_with_UCAC5 got 160792 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 915 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 929 matched stars entering correct_measured_positions(), 156537 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 933 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 156535 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Accuracy estimation diagnostic: 928 matched stars entering correct_measured_positions(), 156536 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.37"
Excluding outliers - 928 stars left (next iteration limit 1021)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits -region wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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.T9PoaS06IK (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits' -> 'wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS_IMAGE_NAME=wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS-calibrated image found: wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Checking if the catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits alredy exist and is non-empty...
Catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat corresponding to the image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
WCS catalog name: wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=18627, passed=162444
Got 162444 stars (including 143508 good ones) from the SExtractor catalog wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat
util/solve_plate_with_UCAC5 got 162444 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.5'
Seting catalog search parameters based on the expected field of view 941.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013076 (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 0.010461 (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 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 920 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.40"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 158932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 609 to 668 (Dec 32.0 to 43.4)
Done reading UCAC5 zone files...
Matched 935 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 158932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.39"
Accuracy estimation diagnostic: 932 matched stars entering correct_measured_positions(), 158932 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.38"
Excluding outliers - 932 stars left (next iteration limit 1025)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits -region wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.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.0YxcosGoU4 (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_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.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_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
Checking if the catalog wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
WCS catalog name: wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=6, blended=12778, passed=95606
Got 95606 stars (including 82764 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits.cat
util/solve_plate_with_UCAC5 got 95606 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 905 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 93481 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 929 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 93481 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.68"
Accuracy estimation diagnostic: 926 matched stars entering correct_measured_positions(), 93481 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 926 stars left (next iteration limit 1018)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits -region wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.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.TJ6kPPRQFq (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_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.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_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
WCS_IMAGE_NAME=wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
WCS-calibrated image found: wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
Checking if the catalog wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits alredy exist and is non-empty...
Catalog wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits.cat corresponding to the image wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
WCS catalog name: wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=12685, passed=96466
Got 96466 stars (including 83704 good ones) from the SExtractor catalog wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits.cat
util/solve_plate_with_UCAC5 got 96466 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 901 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 94587 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Searching UCAC5 zones 611 to 668 (Dec 32.3 to 43.2)
Done reading UCAC5 zone files...
Matched 925 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 94587 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.67"
Accuracy estimation diagnostic: 922 matched stars entering correct_measured_positions(), 94588 with non-zero local correction accuracy
Estimated accuracy of the plate solution: 0.76"
Excluding outliers - 922 stars left (next iteration limit 1014)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits -region wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.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_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.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_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/wcs_Aur-04-Q2b1x1_2026-01-20_23-14-47_20.00sec_-15.00C_LIGHT_0232.fits
Saving fully-calibrated image wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.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_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/wcs_Aur-04-Q2b1x1_2026-01-20_23-15-34_20.00sec_-14.90C_LIGHT_0233.fits
Saving fully-calibrated image wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.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_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-39-51_20.00sec_-5.00C_LIGHT_0413.fits
Saving fully-calibrated image wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.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_2026-04-18_CI_Aur-04-Q2b1x1_224135_TTUQ2b1x1_1421958_9nhd1O8x/wcs_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414.fits
Preparing the HTML report for the field Aur-04-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out183628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183637.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183656.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183661.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183662.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183664.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183670.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out183687.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out198515.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203018.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203526.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out203527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204151.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204643.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out204808.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out35037.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out149329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out183667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out183678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out183693.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out195013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out205082.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
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 183628_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 183628_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:32:43.34 +39:35:35.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.54, MAG_FAINT_SEARCH_LIMIT=15.52)
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Considering the candidate 183637_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 183637_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:46:50.23 +36:28:48.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)
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Considering the candidate 183656_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 183656_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:25:06.01 +34:39:10.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.23, MAG_FAINT_SEARCH_LIMIT=15.21)
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Considering the candidate 183661_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 183661_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:54:11.45 +39:27:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.53, MAG_FAINT_SEARCH_LIMIT=15.51)GAIADR2_OUTPUT=# 0.329 950351128733750912 103.54780185706 +39.45250057480 14.2425 13.5190 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.329#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 183662_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 183662_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:28:41.30 +36:47:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.287 942919941959626496 097.17238686344 +36.79271018084 14.3873 13.7968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.287#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 183664_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 183664_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:49:26.17 +38:57:22.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 1.267 944417304996875008 102.35918744702 +38.95583355647 14.1547 13.5813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.267#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 183665_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 183665_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:52:31.59 +36:33:39.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 183667_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
Preparing report for the candidate 183667_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
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Considering the candidate 183670_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 183670_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:12:21.32 +36:04:50.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)
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Considering the candidate 183674_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 183674_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 183678_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
Preparing report for the candidate 183678_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
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Considering the candidate 183680_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 183680_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:22:11.80 +37:26:37.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 183686_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 183686_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:55:02.04 +34:52:41.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 183687_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 183687_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:28:16.39 +40:36:59.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 2.227 958155427908748416 097.06822749395 +40.61579994752 13.7558 13.1216 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 183691_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 183691_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:49:37.17 +34:06:35.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 183693_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
Preparing report for the candidate 183693_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
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Considering the candidate 183694_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 183694_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:33:06.08 +34:09:31.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 183700_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 183700_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:52:03.67 +39:13:50.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 186131_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 186131_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:50:52.99 +37:33:09.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 188604_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 188604_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:54:03.11 +33:42:14.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189013_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 189013_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:50:16.27 +36:25:14.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 189050_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 189050_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:32:09.85 +34:19:34.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190232_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 190232_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:15:09.20 +39:55:28.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 190383_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 190383_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:50:56.01 +41:47:32.3 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 191271_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 191271_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:17:37.62 +35:07:39.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 191428_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 191428_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:30:53.96 +39:45:26.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193131_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 193131_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:28:04.40 +36:10:59.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193260_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 193260_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:55:07.52 +36:03:46.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193659_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 193659_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:43:22.21 +37:01:28.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193727_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 193727_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:51:24.32 +38:34:44.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193802_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 193802_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:54:03.94 +37:32:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 193941_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 193941_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:44:08.16 +40:14:11.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194481_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 194481_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:37:14.15 +38:26:46.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194486_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 194486_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:52:52.61 +38:52:33.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 194594_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 194594_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:54:01.02 +37:32:21.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194772_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 194772_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:42:21.40 +37:43:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194945_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 194945_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:51:25.67 +41:46:59.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 194973_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 194973_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:38:13.93 +40:38:33.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195006_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 195006_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:15:43.07 +42:02:06.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195013_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
Preparing report for the candidate 195013_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
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Considering the candidate 195225_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 195225_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:40:14.78 +34:55:15.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 195483_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 195483_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:41:34.44 +35:57:40.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 196141_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 196141_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:46:25.52 +35:23:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196219_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 196219_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:50:13.38 +34:12:52.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196228_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 196228_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:30:55.52 +39:45:44.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196387_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 196387_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:55:30.51 +38:58:32.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196413_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 196413_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:30:01.48 +35:49:10.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196424_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 196424_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:15:26.38 +37:22:42.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196536_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 196536_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:46:49.99 +40:15:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196585_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 196585_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:50:57.48 +37:33:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196668_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 196668_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:30:02.21 +35:36:07.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196965_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 196965_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:19:31.48 +37:29:60.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 196987_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 196987_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:52:16.25 +35:09:35.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197509_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 197509_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:34:22.68 +39:27:47.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197653_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 197653_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:47:03.26 +35:26:32.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197808_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 197808_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:50:18.84 +36:25:10.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 197948_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 197948_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:43:55.16 +34:37:55.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198007_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 198007_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:52:06.15 +33:41:52.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198230_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 198230_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:46:14.92 +42:01:51.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198267_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 198267_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:44:06.82 +34:10:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198445_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 198445_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:44:21.45 +40:56:19.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198515_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 198515_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:50:46.41 +34:08:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 1.019 937873286666746880 102.69359411976 +34.13761584163 14.3964 13.9278 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.019#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 198857_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 198857_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:40:17.21 +39:50:55.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198904_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 198904_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:42:25.59 +39:00:59.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 198986_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 198986_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:37:48.18 +35:30:03.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 199299_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 199299_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:30:01.31 +41:16:32.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200087_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 200087_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:48:04.15 +38:03:06.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 200767_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 200767_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:51:43.00 +33:47:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203018_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 203018_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:53:30.61 +34:17:19.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.77, MAG_FAINT_SEARCH_LIMIT=15.75)GAIADR2_OUTPUT=# 1.526 939387795214566272 103.37797609631 +34.28849683309 14.7529 14.0532 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.526#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 203098_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 203098_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:43:27.10 +34:08:37.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 203526_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 203526_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:41:40.95 +34:46:28.8 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.76, MAG_FAINT_SEARCH_LIMIT=15.74)
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Considering the candidate 203527_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 203527_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:51:01.90 +35:32:41.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 1.145 940262422355273216 102.75826134667 +35.54509427275 14.7899 14.1183 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.145#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204151_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 204151_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:52:21.28 +37:05:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.78, MAG_FAINT_SEARCH_LIMIT=15.76)GAIADR2_OUTPUT=# 2.599 941054414324710272 103.08813217299 +37.08436183152 15.0802 14.6541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.599#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 204643_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 204643_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:39:26.37 +41:10:53.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.80, MAG_FAINT_SEARCH_LIMIT=15.78)GAIADR2_OUTPUT=# 0.578 957685524126443008 099.86008826091 +41.18155514582 14.8303 14.1811 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.578#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 204808_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 204808_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:40:27.29 +35:32:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.81, MAG_FAINT_SEARCH_LIMIT=15.79)GAIADR2_OUTPUT=# 0.835 942032636076084864 100.11399309821 +35.54702015079 14.8767 14.3354 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.835#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 205082_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
Preparing report for the candidate 205082_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
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Considering the candidate 58805_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 58805_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:15:09.81 +36:08:52.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 39833_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 39833_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:28:22.27 +35:10:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 141066_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 141066_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:30:55.92 +40:16:59.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 61342_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 61342_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:16:22.38 +36:21:29.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 95476_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 95476_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:21:47.49 +38:33:33.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 53350_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 53350_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:28:01.84 +36:05:01.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 131604_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 131604_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:09:50.71 +40:35:35.8 in the exclusion list exclusion_list.txt ****
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Considering the candidate 33022_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 33022_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:18:22.97 +34:38:17.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 35037_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 35037_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:11:58.40 +34:38:01.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)
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Considering the candidate 127321_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 127321_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks
**** FOUND 06:15:48.74 +41:02:18.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 149329_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
Preparing report for the candidate 149329_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
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Considering the candidate 27922_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414
The candidate 27922_fd_Aur-04-Q2b1x1_2026-04-18_22-40-48_20.00sec_-4.90C_LIGHT_0414 did not pass the final checks