This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
XX Gem,2461118.8222,10.64,0.05,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
XX Gem 20260319.3222 10.64CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:26:13.71 +33:22:24.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3222 2461118.8222 13.88 07:01:53.89 +42:50:13.7
174.08936 19.86512 galactic Aur Second-epoch detections are separated by 6.5" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:01:53.89 +42:50:13.7 (user input) | T | P | (position from user input) J-Ks=2.464+/- (Very red!)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8222,13.88,0.05,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 20260319.3222 13.88CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:01:53.89 +42:50:13.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3222 2461118.8222 13.82 07:01:14.06 +41:55:54.3
174.95421 19.45106 galactic Aur Second-epoch detections are separated by 4.3" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:01:14.06 +41:55:54.3 (user input) | T | P | (position from user input) SpType: DA 2015MNRAS.454.2787G LAMOST J070113.45+415554.6
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8222,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260319.3222 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:01:14.06 +41:55:54.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8222,13.81,0.05,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 20260319.3222 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:00:14.35 +42:06:00.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3222 2461118.8222 13.52 06:58:35.98 +41:19:17.8
175.38614 18.78165 galactic Aur Second-epoch detections are separated by 0.8" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.6528+41.3220 | 06:58:35.98 +41:19:17.8 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6528+41.3220,2461118.8222,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.6528+41.3220 20260319.3222 13.52CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:58:35.98 +41:19:17.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3222 2461118.8222 13.66 06:59:08.79 +42:19:17.7
174.42771 19.21651 galactic Aur Second-epoch detections are separated by 3.9" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.7951+42.3212 | 06:59:08.79 +42:19:17.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.7951+42.3212,2461118.8222,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.7951+42.3212 20260319.3222 13.66CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:59:08.79 +42:19:17.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3222 2461118.8222 13.33 06:58:19.87 +42:35:51.5
174.09891 19.16761 galactic Aur Second-epoch detections are separated by 0.7" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:58:19.87 +42:35:51.5 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8222,13.33,0.05,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 20260319.3222 13.33CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:58:19.87 +42:35:51.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3222 2461118.8222 13.17 06:57:32.50 +42:44:55.2
173.89667 19.08182 galactic Aur Second-epoch detections are separated by 0.5" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 951340994140632448 | 06:57:33.14 +42:44:53.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 951340994140632448,2461118.8222,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 951340994140632448 20260319.3222 13.17CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:57:32.50 +42:44:55.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3222 2461118.8222 13.13 06:58:13.71 +41:43:43.1
174.95693 18.85544 galactic Aur Second-epoch detections are separated by 1.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 951184661627764224 | 06:58:12.99 +41:43:46.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 951184661627764224,2461118.8222,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 951184661627764224 20260319.3222 13.13CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:58:13.71 +41:43:43.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8222,13.83,0.05,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 20260319.3222 13.83CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:26:18.92 +36:57:05.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461118.8222,14.42,0.05,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 20260319.3222 14.42CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:44:44.69 +34:38:04.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3222 2461118.8222 13.32 08:16:27.06 +40:19:20.8
180.59256 32.75356 galactic Lyn Second-epoch detections are separated by 0.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:16:27.06 +40:19:20.8 (user input) | T | P | (position from user input) J-Ks=0.498+/-0.025 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8222,13.32,0.05,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 20260319.3222 13.32CV 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
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:16:27.06 +40:19:20.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461118.8222,12.74,0.05,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 20260319.3222 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:03:09.32 +33:48:08.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20_00sec_-15_00C_LIGHT_0043_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20_00sec_-14_90C_LIGHT_0042_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.89788103 23.12.2025 09:32:46.921 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
First image: 2461032.89788103 23.12.2025 09:32:46.921 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Last image: 2461118.82252444 19.03.2026 07:44:16.112 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 5
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.49
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): 16340
Objects passed selection criteria: 16327
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 15127.8
Average stars matched: 14863.5 (98.2532 %)
Memory usage VmPeak: 121328 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 02:51:32 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: 2461032.89788103 23.12.2025 09:32:46.921 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
First image: 2461032.89788103 23.12.2025 09:32:46.921 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Last image: 2461118.82252444 19.03.2026 07:44:16.112 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 133
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
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: 38 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): 93774
Objects passed selection criteria: 93589
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 84768
Average stars matched: 82414.8 (97.2239 %)
Memory usage VmPeak: 1925644 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 02:53:14 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
SExtractor catalog cache: saved Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat to cache
SExtractor catalog cache: saved Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.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: 2461118.82192103
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'
Plate-solving the images
wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits exists and is non-empty
Saving wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits to local_wcs_cache/
'wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits' -> 'local_wcs_cache/wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits'
wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits exists and is non-empty
Saving wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits to local_wcs_cache/
'wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits' -> 'local_wcs_cache/wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits'
wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
Saving wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits to local_wcs_cache/
'wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits' -> 'local_wcs_cache/wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits'
wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
Saving wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits to local_wcs_cache/
'wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits' -> 'local_wcs_cache/wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:38:10.768 +37:59:37.83
Second-epoch image center 07:38:06.471 +38:02:50.15
Angular distance between the image centers 0.06 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:38:10.768 +37:59:37.83
Second-epoch image center 07:38:09.321 +38:02:50.08
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 07:38:06.471 +38:02:50.15
Second-epoch second image center 07:38:09.321 +38:02:50.08
Angular distance between the image centers 0.00935 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits &> /tmp/tmp.BXCJQZrgv4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits &> /tmp/tmp.mNAAIHgitT
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.VwoIgskdxd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.kg6rSJHYOF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
Found non-empty wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
The reference image (wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits) and catalog (wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat) found
'wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 7689 out of 17251 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.958948
a=0.000000 b=1.000000 c=22.958948
From vast_summary.log: estimated ref. image limiting mag.: -7.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 1 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
2.2 pix Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
2.5 pix fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
2.5 pix fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
Limiting magnitude estimates:
15.5 mag. Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
15.5 mag. Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
15.0 mag. fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
15.0 mag. fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.2 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.BXCJQZrgv4 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.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_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits' -> 'wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS-calibrated image found: wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Checking if the catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS catalog name: wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1370, passed=17251
Got 17251 stars (including 15857 good ones) from the SExtractor catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
util/solve_plate_with_UCAC5 got 17251 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
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...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits -region wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.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.mNAAIHgitT (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.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_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits' -> 'wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS-calibrated image found: wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Checking if the catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS catalog name: wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1310, passed=17199
Got 17199 stars (including 15864 good ones) from the SExtractor catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat
util/solve_plate_with_UCAC5 got 17199 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
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...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits -region wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.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.VwoIgskdxd (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_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.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_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=747, passed=13239
Got 13239 stars (including 12483 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 13239 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
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...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.58"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.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.kg6rSJHYOF (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_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.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_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=784, passed=13193
Got 13193 stars (including 12401 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 13193 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
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...
Done reading UCAC5 zone files...
Matched 955 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 955 stars left (next iteration limit 1050)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits'
Saving fully-calibrated image wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits'
Saving fully-calibrated image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits'
Saving fully-calibrated image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits'
Preparing the HTML report for the field Lyn-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out14539.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 5s
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 14539_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
Preparing report for the candidate 14539_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 6s
Prepared the HTML report for the field Lyn-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:26:13.71 +33:22:24.3
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
SExtractor catalog cache: saved Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat to cache
SExtractor catalog cache: saved Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Creating symlink local_wcs_cache/wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits exists and is non-empty
wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits exists and is non-empty
wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits exists and is non-empty
wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:38:10.768 +37:59:37.83
Second-epoch image center 07:38:06.471 +38:02:50.15
Angular distance between the image centers 0.06 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:38:10.768 +37:59:37.83
Second-epoch image center 07:38:09.321 +38:02:50.08
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 07:38:06.471 +38:02:50.15
Second-epoch second image center 07:38:09.321 +38:02:50.08
Angular distance between the image centers 0.00935 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits &> /tmp/tmp.0X1vL6YeME
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits &> /tmp/tmp.owA6sg8rNY
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits &> /tmp/tmp.M7tzDOav6h
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits &> /tmp/tmp.zdcEO4PnvY
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
Found non-empty wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
The reference image (wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits) and catalog (wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat) found
'wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat' -> 'wcsmag.cat'
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
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 7746 out of 100375 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.850461
a=0.000000 b=1.000000 c=22.850461
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.61
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.61
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 78 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
2.0 pix Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
2.4 pix fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
2.4 pix fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
Limiting magnitude estimates:
15.6 mag. Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
15.6 mag. Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
15.1 mag. fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
15.1 mag. fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.0X1vL6YeME (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.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_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits' -> 'wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS-calibrated image found: wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Checking if the catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS catalog name: wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=7665, passed=100350
Got 100350 stars (including 92512 good ones) from the SExtractor catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
util/solve_plate_with_UCAC5 got 100350 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
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...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits -region wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.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.owA6sg8rNY (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.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_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits' -> 'wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS-calibrated image found: wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Checking if the catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS catalog name: wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=7582, passed=100415
Got 100415 stars (including 92657 good ones) from the SExtractor catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat
util/solve_plate_with_UCAC5 got 100415 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (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 0.010459 (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...
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits -region wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.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.M7tzDOav6h (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_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.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_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
Checking if the catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
WCS catalog name: wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=29, blended=4793, passed=70211
Got 70211 stars (including 65342 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits.cat
util/solve_plate_with_UCAC5 got 70211 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.52"
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...
Done reading UCAC5 zone files...
Matched 954 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.52"
Estimated accuracy of the plate solution: 0.54"
Excluding outliers - 954 stars left (next iteration limit 1049)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits -region wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.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.zdcEO4PnvY (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_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.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_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
Checking if the catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
WCS catalog name: wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=4733, passed=70463
Got 70463 stars (including 65636 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits.cat
util/solve_plate_with_UCAC5 got 70463 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.7'
Seting catalog search parameters based on the expected field of view 937.7 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013024 (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 0.010419 (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...
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
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...
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits -region wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.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_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Saving fully-calibrated image wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.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_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Saving fully-calibrated image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.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_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-43-23_20.00sec_-14.90C_LIGHT_0042.fits
Saving fully-calibrated image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.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_2026-03-19_CI_Lyn-05-Q2b1x1_024606_TTUQ2b1x1_28990_zX5iePZK/wcs_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043.fits
Preparing the HTML report for the field Lyn-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out110559.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118033.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118047.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118050.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118051.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118056.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118064.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118069.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118084.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118087.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118098.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118103.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118121.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118122.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118124.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118133.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118134.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118138.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118139.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118146.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118155.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118190.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118302.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118329.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118387.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118400.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118420.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118430.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118453.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118463.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118506.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118522.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118545.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118558.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118563.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118596.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118613.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118640.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118648.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118655.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118666.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118709.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118738.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118745.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out27619.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out118042.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out118068.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out118060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118117.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118704.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out76980.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 30s
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: 6s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118029_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118029_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 08:16:05.44 +39:07:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 0.592 909177235772103552 124.02245714091 +39.12696940534 14.3512 13.6818 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118032_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118032_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 08:17:53.61 +41:41:34.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 1.240 915671913518291584 124.47295782159 +41.69279767002 14.2655 13.7213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118033_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118033_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:57:12.60 +32:52:13.5 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118042_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118042_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:07:54.93 +37:42:42.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118047_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118047_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 06:59:55.92 +39:46:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 1.044 950410120108996224 104.98264109609 +39.76999411122 13.4443 12.8626 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.044#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118050_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118050_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:00:15.60 +40:28:32.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 3.227 950468054923481344 105.06383182567 +40.47581147626 13.6800 13.1991 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118051_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118051_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 06:59:57.22 +39:08:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 1.069 947284900042054144 104.98805261785 +39.14135265911 13.3886 12.6847 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.069#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118053_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118053_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:14:28.13 +36:37:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 0.117 897832680955293696 108.61719967044 +36.63192060420 14.1601 13.4250 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.117#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118056_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118056_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 08:11:03.04 +37:48:19.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.92, MAG_FAINT_SEARCH_LIMIT=14.90)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118058_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118058_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:01:04.88 +33:21:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.640 891088482790189952 105.27060579851 +33.36320033401 13.1289 12.5842 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118060_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
Preparing report for the candidate 118060_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118064_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118064_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 08:17:41.83 +39:04:28.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 2.378 908445888740971392 124.42345880301 +39.07469106444 14.2027 13.9677 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.378#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118068_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118068_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 08:10:15.25 +33:57:25.2 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118069_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118069_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 06:59:50.96 +36:14:23.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 3.052 940061898921651328 104.96171309273 +36.23909316026 13.2665 12.5098 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.052#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118075_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118075_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 08:19:18.21 +41:44:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 1.795 915681671683969664 124.82527796138 +41.73991512131 14.0359 13.5782 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.795#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118076_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118076_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:01:39.14 +34:19:49.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 3.883 939564954025618688 105.41177721516 +34.33040263045 13.6632 13.1773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.883#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118082_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
Preparing report for the candidate 118082_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118084_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118084_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:07:22.63 +35:38:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 4.750 891712524357443456 106.84315166637 +35.64535615400 13.6180 13.0417 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.750#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118086_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118086_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 06:59:50.17 +42:25:38.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 4.776 951276951885211392 104.95724442031 +42.42746648559 13.2880 12.8227 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.776#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118087_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118087_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 06:59:17.98 +41:23:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 5.058 951118274316785408 104.82304527145 +41.38721905052 13.0051 12.2543 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118098_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118098_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:00:40.36 +42:34:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 4.121 951299487576923392 105.16944509941 +42.57542912035 13.0143 12.5332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118099_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118099_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:19:58.40 +39:38:16.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.778 948074349390826368 109.99390108491 +39.63754788527 13.8934 13.2111 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.778#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118103_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118103_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:01:36.83 +36:12:30.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 2.107 940016711570573568 105.40282460083 +36.20804877219 13.1543 12.6069 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.107#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118110_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
Preparing report for the candidate 118110_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118111_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
Preparing report for the candidate 118111_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118117_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
Preparing report for the candidate 118117_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118121_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118121_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 06:58:09.40 +42:04:51.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.263 951215791550586752 104.53869904136 +42.08092081053 12.5447 11.8410 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.263#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118122_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118122_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 06:58:08.90 +41:29:13.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 3.871 951129303792799232 104.53847340031 +41.48740660898 12.8093 12.3409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.871#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118123_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
Preparing report for the candidate 118123_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118124_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118124_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:03:18.19 +42:40:07.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 5.277 952606227082791040 105.82777586443 +42.66880835432 12.7550 12.0531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118133_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118133_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:28:16.02 +33:29:27.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.31, MAG_FAINT_SEARCH_LIMIT=14.29)GAIADR2_OUTPUT=# 1.751 893492187006085888 112.06704788504 +33.49047082790 13.3737 12.6937 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.751#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118134_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118134_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 06:59:30.68 +40:27:45.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 5.114 950509797709452416 104.87960203297 +40.46215597040 12.5779 12.1352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.114#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118137_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118137_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 06:59:05.69 +41:43:51.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.18, MAG_FAINT_SEARCH_LIMIT=14.16)GAIADR2_OUTPUT=# 2.888 951138619578328064 104.77477117471 +41.73098183187 12.7536 12.3704 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118138_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118138_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:00:07.26 +41:39:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 2.482 951145594605299456 105.03052165908 +41.66490891625 12.5465 11.9409 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.482#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118139_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118139_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:02:07.02 +36:32:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 4.566 940092238570691584 105.52784962746 +36.53794675616 13.3200 12.8276 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.566#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118145_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
Preparing report for the candidate 118145_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118146_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118146_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 06:59:16.77 +41:41:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 2.721 951137520066699776 104.82088330609 +41.68526078807 12.4104 11.9933 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.721#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118147_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
Preparing report for the candidate 118147_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118152_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118152_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 06:58:01.69 +41:15:45.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 3.076 950747360941089152 104.50817213866 +41.26243751284 11.9079 11.2044 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118155_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118155_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 06:57:49.08 +42:33:25.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 2.563 951334637589037440 104.45546347537 +42.55705763138 11.7208 10.9745 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.563#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118157_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118157_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:00:03.39 +42:22:12.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.29, MAG_FAINT_SEARCH_LIMIT=13.27)GAIADR2_OUTPUT=# 1.392 951276569631435648 105.01463939543 +42.37015526699 11.6089 10.8848 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118190_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118190_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 08:01:58.04 +34:06:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 0.660 905546648377001984 120.49179977544 +34.10623682694 11.2918 10.9272 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118247_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118247_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:19:35.70 +34:28:21.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 0.345 896647957177334528 109.89884268176 +34.47255349015 12.2848 11.6083 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.345#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118302_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118302_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:26:05.93 +35:38:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.00, MAG_FAINT_SEARCH_LIMIT=13.98)GAIADR2_OUTPUT=# 0.639 897003889706563456 111.52483393525 +35.64311731153 12.9840 12.5307 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.639#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118329_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118329_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 08:07:53.09 +38:35:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.178 908925825566745216 121.97161623312 +38.59812950737 12.9369 12.2797 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118349_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118349_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:24:42.28 +41:58:52.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.27, MAG_FAINT_SEARCH_LIMIT=14.25)GAIADR2_OUTPUT=# 1.756 948808101603537920 111.17575090495 +41.98159954201 13.2250 12.5465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118357_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118357_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:15:33.87 +42:05:04.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.33, MAG_FAINT_SEARCH_LIMIT=14.31)GAIADR2_OUTPUT=# 4.595 949387097554874624 108.89127104761 +42.08322834745 13.3946 12.8960 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.595#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118376_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118376_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:05:55.48 +33:43:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.32, MAG_FAINT_SEARCH_LIMIT=14.30)GAIADR2_OUTPUT=# 0.996 891252000785047936 106.48109695273 +33.72228500280 13.3347 12.8416 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118387_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118387_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:23:15.83 +35:10:43.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.402 896880194648481024 110.81579219150 +35.17908721532 13.3992 12.8456 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.402#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118400_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118400_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:02:43.56 +32:46:17.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.45, MAG_FAINT_SEARCH_LIMIT=14.43)GAIADR2_OUTPUT=# 4.719 890818896282768896 105.68056382845 +32.77047973489 13.0844 12.4146 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.719#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118420_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118420_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:17:44.05 +34:07:16.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 0.264 896537284460202624 109.43358031070 +34.12110073568 13.8089 13.3953 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.264#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118430_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118430_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:55:55.70 +38:04:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 1.270 919393863457842176 118.98239352671 +38.07489354836 13.6625 13.0419 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.270#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118431_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118431_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:08:26.86 +33:15:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.58, MAG_FAINT_SEARCH_LIMIT=14.56)GAIADR2_OUTPUT=# 2.584 891165964000305024 107.11238212155 +33.25670236122 13.5543 12.9012 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.584#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118450_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118450_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:06:07.51 +34:26:29.4 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118453_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118453_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:07:56.04 +41:39:44.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.74, MAG_FAINT_SEARCH_LIMIT=14.72)GAIADR2_OUTPUT=# 0.690 948003018573655040 106.98348342990 +41.66246895834 13.6681 13.2133 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.690#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118454_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118454_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:30:56.11 +40:21:33.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 0.806 900393271737701120 112.73354079356 +40.35939422010 13.6931 13.0375 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.806#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118463_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118463_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:21:01.80 +35:19:17.9 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118491_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
Preparing report for the candidate 118491_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118506_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118506_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:30:03.84 +33:32:02.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 1.467 893507167851961728 112.51555983364 +33.53382301022 13.8767 13.0675 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118522_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118522_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:42:50.08 +33:24:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 0.926 894006964606278912 115.70896259222 +33.40865467091 13.9734 13.2792 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.926#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118545_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118545_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:18:34.60 +42:03:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 2.599 949700733246308736 109.64320187003 +42.05217354372 14.0827 13.5089 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#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118558_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118558_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:23:19.58 +33:09:35.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.90, MAG_FAINT_SEARCH_LIMIT=14.88)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118563_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118563_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:47:08.27 +41:58:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.05, MAG_FAINT_SEARCH_LIMIT=15.03)GAIADR2_OUTPUT=# 3.022 924225839104802688 116.78553046925 +41.97762524857 14.3430 13.8264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118596_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118596_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:28:35.66 +41:58:11.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.14, MAG_FAINT_SEARCH_LIMIT=15.12)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118613_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118613_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:43:56.60 +38:01:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.193 920143008834162048 115.98551116947 +38.02218541833 14.6055 14.1424 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.193#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118640_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118640_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:38:34.34 +41:15:44.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 2.112 924511334171006336 114.64332907851 +41.26297336924 14.3793 13.7372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118648_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118648_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:45:01.81 +40:43:23.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.24, MAG_FAINT_SEARCH_LIMIT=15.22)GAIADR2_OUTPUT=# 0.347 923500401948731904 116.25757723762 +40.72337028899 14.2625 13.8418 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.347#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118655_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118655_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:57:36.36 +40:03:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 2.674 919857341968609792 119.40153582409 +40.05396447670 14.4910 13.9671 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.674#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118666_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118666_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:32:05.09 +39:11:29.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 0.865 899444010950350592 113.02096297376 +39.19173017517 14.6918 14.1628 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.865#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118704_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
Preparing report for the candidate 118704_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118709_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118709_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:22:33.56 +35:54:26.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 4.971 897128684276493952 110.64078165849 +35.90859182982 15.0634 14.4656 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.971#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118738_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118738_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:32:53.29 +39:51:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 2.160 900312388913733120 113.22270967156 +39.85770047833 14.6148 13.9531 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.160#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118745_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 118745_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:34:56.63 +35:45:53.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20114_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
Preparing report for the candidate 20114_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27619_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 27619_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 08:11:44.39 +39:38:26.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.55, MAG_FAINT_SEARCH_LIMIT=13.53)GAIADR2_OUTPUT=# 3.998 909451357764900352 122.93351895034 +39.64065323809 12.6483 12.2038 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 110559_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 110559_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks
**** FOUND 07:00:24.35 +35:57:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 4.147 939914358205030912 105.10033946115 +35.95423260620 13.6221 13.0572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.147#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 76980_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
Preparing report for the candidate 76980_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64977_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043
The candidate 64977_fd_Lyn-05-Q2b1x1_2026-03-19_02-44-16_20.00sec_-15.00C_LIGHT_0043 did not pass the final checks