This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz
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
AA Aur,2461118.8245,10.34,0.05,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
AA Aur 20260319.3245 10.34CV 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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:41:13.10 +44:10:01.1 ;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-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_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,2461118.8245,14.47,0.05,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 20260319.3245 14.47CV 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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:30:35.57 +49:28:22.2 ;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-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_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
Gaia DR3 968164965154602368,2461118.8245,14.01,0.05,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 968164965154602368 20260319.3245 14.01CV 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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:02.26 +50:18:32.1 ;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-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3245 2461118.8245 13.33 06:25:05.06 +49:36:58.0
165.05181 16.33018 galactic Aur Second-epoch detections are separated by 2.7" and 4.9 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 | 06:25:05.06 +49:36:58.0 (user input) | T | P | (position from user input) 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
target,2461118.8245,13.33,0.05,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 20260319.3245 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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:05.06 +49:36:58.0 ;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-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3245 2461118.8245 13.47 06:27:38.25 +49:49:11.0
165.02148 16.78944 galactic Aur Second-epoch detections are separated by 6.1" and 3.3 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 968090679400665216 | 06:27:38.78 +49:48:34.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
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 968090679400665216,2461118.8245,13.47,0.05,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 968090679400665216 20260319.3245 13.47CV 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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:38.25 +49:49:11.0 ;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-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3245 2461118.8245 13.49 06:25:52.57 +50:26:36.4
164.30682 16.76683 galactic Aur Second-epoch detections are separated by 3.6" and 3.9 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 J096.4698+50.4415 | 06:25:52.57 +50:26:36.4 (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 J096.4698+50.4415,2461118.8245,13.49,0.05,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 J096.4698+50.4415 20260319.3245 13.49CV 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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:52.57 +50:26:36.4 ;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-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 19.3245 2461118.8245 13.16 06:25:53.98 +50:24:22.8
164.34411 16.75607 galactic Aur Second-epoch detections are separated by 4.5" and 4.3 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 971131486182684800 | 06:25:53.06 +50:24:25.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
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 971131486182684800,2461118.8245,13.16,0.05,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 971131486182684800 20260319.3245 13.16CV 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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:53.98 +50:24:22.8 ;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-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_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,2461118.8245,14.12,0.05,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 20260319.3245 14.12CV 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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:44:07.59 +40:52:27.5 ;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-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_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
NSVS J0721093+454816,2461118.8245,11.62,0.05,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
NSVS J0721093+454816 20260319.3245 11.62CV 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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:21:09.47 +45:48:14.3 ;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-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_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
EP Lyn,2461118.8245,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
EP Lyn 20260319.3245 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:12:18.81 +47:19:32.9 ;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-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20_00sec_-15_00C_LIGHT_0047_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20_00sec_-15_00C_LIGHT_0486_fits__*pix.png resample_wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20_00sec_-15_00C_LIGHT_0046_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: 2461032.89011257 23.12.2025 09:21:35.726 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
First image: 2461032.89011257 23.12.2025 09:21:35.726 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
Last image: 2461118.82481519 19.03.2026 07:47:34.032 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.51
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 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): 17174
Objects passed selection criteria: 17155
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: 15525.2
Average stars matched: 15224.5 (98.0628 %)
Memory usage VmPeak: 121948 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 03:22:02 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: 2461032.89011257 23.12.2025 09:21:35.726 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
First image: 2461032.89011257 23.12.2025 09:21:35.726 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
Last image: 2461118.82481519 19.03.2026 07:47:34.032 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 158
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.27
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: 29 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): 99165
Objects passed selection criteria: 99011
Measurements per detected object (mean, median, min, max): 3.4 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.4 4.0 2 4
Average stars detected per image: 88752.8
Average stars matched: 86155.5 (97.0736 %)
Memory usage VmPeak: 1995624 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 03:23:23 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
SExtractor catalog cache: saved Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat to cache
SExtractor catalog cache: saved Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.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: 2461118.82424372
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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits exists and is non-empty
Saving wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits to local_wcs_cache/
'wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits' -> 'local_wcs_cache/wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits'
wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits exists and is non-empty
Saving wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits to local_wcs_cache/
'wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits' -> 'local_wcs_cache/wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits'
wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits exists and is non-empty
Saving wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits to local_wcs_cache/
'wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits' -> 'local_wcs_cache/wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits'
wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits exists and is non-empty
Saving wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits to local_wcs_cache/
'wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits' -> 'local_wcs_cache/wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.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 07:11:59.469 +45:59:48.78
Second-epoch image center 07:12:11.623 +45:59:52.49
Angular distance between the image centers 0.04 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 07:11:59.469 +45:59:48.78
Second-epoch image center 07:12:09.019 +45:59:53.78
Angular distance between the image centers 0.03 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 07:12:11.623 +45:59:52.49
Second-epoch second image center 07:12:09.019 +45:59:53.78
Angular distance between the image centers 0.00755 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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits &> /tmp/tmp.6NUpSRSn7g
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits &> /tmp/tmp.2RqJm0rJc9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits &> /tmp/tmp.lcYKk89Jrx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits &> /tmp/tmp.CtQdlEnJS9
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits and wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits and wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat
Found non-empty wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits and wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat
The reference image (wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits) and catalog (wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat) found
'wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.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 6450 out of 18061 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.995538
a=0.000000 b=1.000000 c=22.995538
From vast_summary.log: estimated ref. image limiting mag.: -7.51
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.49
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.49
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 3 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
2.2 pix Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
2.5 pix fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
2.5 pix fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
Limiting magnitude estimates:
15.5 mag. Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
15.5 mag. Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
15.0 mag. fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
15.0 mag. fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.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.6NUpSRSn7g (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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits' -> 'wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
WCS_IMAGE_NAME=wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
WCS-calibrated image found: wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
Checking if the catalog wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat corresponding to the image wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits alredy exist and is non-empty...
Catalog wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat corresponding to the image wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
WCS catalog name: wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1313, passed=18061
Got 18061 stars (including 16725 good ones) from the SExtractor catalog wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat
util/solve_plate_with_UCAC5 got 18061 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 943 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: 0.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.30"
Estimated accuracy of the plate solution: 0.30"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits -region wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.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.2RqJm0rJc9 (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-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.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-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.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-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits' -> 'wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
WCS_IMAGE_NAME=wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
WCS-calibrated image found: wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
Checking if the catalog wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits.cat corresponding to the image wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits alredy exist and is non-empty...
Catalog wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits.cat corresponding to the image wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
WCS catalog name: wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1293, passed=17960
Got 17960 stars (including 16635 good ones) from the SExtractor catalog wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits.cat
util/solve_plate_with_UCAC5 got 17960 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 944 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: 0.32"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.30"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 944 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.31"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 944 stars left (next iteration limit 1038)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits -region wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.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.lcYKk89Jrx (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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
WCS-calibrated image found: wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
Checking if the catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits.cat corresponding to the image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits.cat corresponding to the image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
WCS catalog name: wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=794, passed=13201
Got 13201 stars (including 12402 good ones) from the SExtractor catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits.cat
util/solve_plate_with_UCAC5 got 13201 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 942 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: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
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 942 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.61"
Excluding outliers - 942 stars left (next iteration limit 1036)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits -region wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.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.CtQdlEnJS9 (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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
WCS-calibrated image found: wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
Checking if the catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits.cat corresponding to the image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits.cat corresponding to the image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
WCS catalog name: wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=786, passed=13266
Got 13266 stars (including 12472 good ones) from the SExtractor catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits.cat
util/solve_plate_with_UCAC5 got 13266 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 940 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: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
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 940 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.60"
Excluding outliers - 940 stars left (next iteration limit 1034)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits -region wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits'
Saving fully-calibrated image wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits'
Saving fully-calibrated image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits'
Saving fully-calibrated image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits'
Preparing the HTML report for the field Lyn-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20960.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out11459.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
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 20960_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 20960_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:58:43.69 +47:38:57.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.48, MAG_FAINT_SEARCH_LIMIT=12.46)GAIADR2_OUTPUT=# 0.534 978530890199346688 104.68223283657 +47.64924026428 11.4030 10.9209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.534#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21040_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 21040_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:21:09.50 +45:48:14.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.47, MAG_FAINT_SEARCH_LIMIT=12.45)GAIADR2_OUTPUT=# 1.018 974551654540475648 110.28997179198 +45.80391898286 10.5651 9.0037 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.018#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 11459_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
Preparing report for the candidate 11459_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 4s
Prepared the HTML report for the field Lyn-03-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 ####
06:41:13.10 +44:10:01.1
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
SExtractor catalog cache: saved Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat to cache
SExtractor catalog cache: saved Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
Creating symlink local_wcs_cache/wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits exists and is non-empty
wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits exists and is non-empty
wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits exists and is non-empty
wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.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 07:11:59.469 +45:59:48.78
Second-epoch image center 07:12:11.623 +45:59:52.49
Angular distance between the image centers 0.04 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 07:11:59.469 +45:59:48.78
Second-epoch image center 07:12:09.019 +45:59:53.78
Angular distance between the image centers 0.03 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 07:12:11.623 +45:59:52.49
Second-epoch second image center 07:12:09.019 +45:59:53.78
Angular distance between the image centers 0.00755 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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits &> /tmp/tmp.N4uWrv2KAc
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits &> /tmp/tmp.2GzSRl8vMf
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits &> /tmp/tmp.k9y0vCIMn0
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits &> /tmp/tmp.9iQjiqcJgy
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits and wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits and wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat
Found non-empty wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits and wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat
The reference image (wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits) and catalog (wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat) found
'wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.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 6474 out of 105943 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.891349
a=0.000000 b=1.000000 c=22.891349
From vast_summary.log: estimated ref. image limiting mag.: -7.27
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.62
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.62
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 96 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
2.1 pix Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
2.4 pix fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
2.4 pix fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
Limiting magnitude estimates:
15.6 mag. Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
15.6 mag. Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
15.1 mag. fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
15.1 mag. fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 14.5 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.N4uWrv2KAc (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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits' -> 'wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
WCS_IMAGE_NAME=wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
WCS-calibrated image found: wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
Checking if the catalog wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat corresponding to the image wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits alredy exist and is non-empty...
Catalog wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat corresponding to the image wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
WCS catalog name: wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=8312, passed=105920
Got 105920 stars (including 97438 good ones) from the SExtractor catalog wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat
util/solve_plate_with_UCAC5 got 105920 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 946 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: 0.32"
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 946 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 - 946 stars left (next iteration limit 1040)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits -region wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.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.2GzSRl8vMf (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-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.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-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.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-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits' -> 'wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
WCS_IMAGE_NAME=wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
WCS-calibrated image found: wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
Checking if the catalog wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits.cat corresponding to the image wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits alredy exist and is non-empty...
Catalog wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits.cat corresponding to the image wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
WCS catalog name: wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=21, blended=8212, passed=105795
Got 105795 stars (including 97423 good ones) from the SExtractor catalog wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits.cat
util/solve_plate_with_UCAC5 got 105795 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 948 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: 0.33"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 948 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.33"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 948 stars left (next iteration limit 1042)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits -region wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.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.k9y0vCIMn0 (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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
WCS-calibrated image found: wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
Checking if the catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits.cat corresponding to the image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits.cat corresponding to the image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
WCS catalog name: wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=5014, passed=73480
Got 73480 stars (including 68390 good ones) from the SExtractor catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits.cat
util/solve_plate_with_UCAC5 got 73480 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 941 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: 0.60"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.55"
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 941 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.55"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 941 stars left (next iteration limit 1035)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits -region wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.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.9iQjiqcJgy (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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
WCS-calibrated image found: wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
Checking if the catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits.cat corresponding to the image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits.cat corresponding to the image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
WCS catalog name: wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=19, blended=4805, passed=72203
Got 72203 stars (including 67318 good ones) from the SExtractor catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits.cat
util/solve_plate_with_UCAC5 got 72203 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.9'
Seting catalog search parameters based on the expected field of view 937.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013026 (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 0.010421 (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 943 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: 0.59"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.56"
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 943 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.56"
Estimated accuracy of the plate solution: 0.57"
Excluding outliers - 943 stars left (next iteration limit 1037)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits -region wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.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-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/wcs_Lyn-03-Q2b1x1_2025-12-23_03-21-35_20.00sec_-15.00C_LIGHT_0486.fits
Saving fully-calibrated image wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/wcs_Lyn-03-Q2b1x1_2025-12-23_03-22-40_20.00sec_-14.90C_LIGHT_0487.fits
Saving fully-calibrated image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-46-44_20.00sec_-15.00C_LIGHT_0046.fits
Saving fully-calibrated image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.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-03-Q2b1x1_031948_TTUQ2b1x1_31218_WnBZjiTz/wcs_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047.fits
Preparing the HTML report for the field Lyn-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out116159.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out116292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out123985.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out123994.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out123999.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124007.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124008.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124010.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124016.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124017.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124024.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124034.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124037.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124067.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124069.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124081.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124088.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124095.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124104.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124107.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124115.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124116.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124129.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124139.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124140.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124148.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124150.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124164.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124169.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124184.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124475.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124489.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124587.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124620.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124660.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124676.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124684.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124818.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124819.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124836.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124864.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124932.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124938.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124947.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124949.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124983.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125041.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125079.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125099.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125108.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125143.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125157.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125167.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out24471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out86737.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out124061.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out124941.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out123987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out125011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out37718.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out52210.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 18s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 5s
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Considering the candidate 123985_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 123985_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:30:08.51 +43:58:16.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 5.286 958978481081787648 097.53745595551 +43.97092430570 13.7588 13.1647 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.286#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 123987_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
Preparing report for the candidate 123987_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
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Considering the candidate 123994_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 123994_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:48:36.95 +45:03:40.7 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)
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Considering the candidate 123999_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 123999_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:01:27.74 +44:23:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 1.998 953044206371961600 105.36634486968 +44.39097361603 14.3255 13.7845 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124007_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124007_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:36:38.59 +46:01:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 0.661 975176447725439488 114.16102684613 +46.02697171060 14.3389 13.5266 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124008_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124008_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:03:01.31 +47:23:32.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 2.178 978547829551245312 105.75619449224 +47.39187938320 14.1967 13.7526 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.178#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124010_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124010_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:59:52.00 +46:58:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.351 978430658546501376 104.96717159563 +46.97551770239 14.2725 13.6486 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124011_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124011_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 124016_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124016_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:32:08.84 +49:02:37.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 0.987 967993995393444608 098.03715908322 +49.04343915955 13.4522 13.0045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.987#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124017_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124017_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:56:34.82 +43:08:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.11, MAG_FAINT_SEARCH_LIMIT=15.09)GAIADR2_OUTPUT=# 1.301 952106361608657664 104.14504734921 +43.14750076877 14.0288 13.2865 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.301#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124024_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124024_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:34:38.18 +41:00:22.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 5.002 957493315750147584 098.66084996795 +41.00666882210 13.4731 12.9610 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.002#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124027_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124027_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:35:58.20 +50:47:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.084 992031552959228288 098.99297271828 +50.79551000225 13.3321 12.6542 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.084#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124028_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124028_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:37:36.61 +41:06:56.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 0.852 924415711019517696 114.40285458436 +41.11560442898 14.2013 13.6432 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.852#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124034_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124034_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:38:18.20 +43:29:00.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 1.320 925256528177033216 114.57616592753 +43.48311300839 13.8343 13.3173 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.320#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124037_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124037_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:58:29.02 +49:35:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 1.723 934117011348445952 119.62162576394 +49.59888335427 13.9690 13.4624 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.723#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124040_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124040_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:29:06.07 +47:16:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 2.390 965938557187854848 097.27595409199 +47.26846068521 13.1293 12.3619 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.390#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124042_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
Preparing report for the candidate 124042_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
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Considering the candidate 124055_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124055_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:32:14.24 +41:21:59.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 5.770 957542480239145088 098.05805326904 +41.36521700392 13.1453 12.3895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.770#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124057_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124057_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:33:02.61 +41:05:50.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.82, MAG_FAINT_SEARCH_LIMIT=14.80)GAIADR2_OUTPUT=# 2.869 957523414880988288 098.26176887075 +41.09701872614 13.5402 13.0844 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124061_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124061_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:42:34.73 +40:45:19.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)
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Considering the candidate 124065_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124065_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:32:27.32 +50:01:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 4.056 968146655710965248 098.11552791976 +50.03026294263 13.0028 12.2777 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.056#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124067_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124067_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:27:15.52 +47:39:26.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 4.088 965994838438778880 096.81589044551 +47.65652457278 13.1162 12.5813 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.088#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124069_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124069_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:09:09.12 +44:19:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.275 953136775803345664 107.28833517070 +44.31895505958 14.1112 13.6261 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.275#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124077_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124077_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:27:51.78 +50:18:08.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.68, MAG_FAINT_SEARCH_LIMIT=14.66)GAIADR2_OUTPUT=# 2.440 968130987670006272 096.96473657171 +50.30224346137 12.8316 12.1978 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.440#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124079_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124079_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:15:50.99 +41:03:08.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 1.364 949274638131375488 108.96208998874 +41.05207582701 13.8577 13.0209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.364#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124080_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124080_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 124081_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124081_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:33:23.13 +40:40:53.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 1.754 957458990371696512 098.34631251381 +40.68104289476 12.9808 12.3908 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124088_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124088_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:34:58.27 +40:55:03.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 4.911 957480426552107904 098.74455291237 +40.91782744129 13.0091 12.4628 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124095_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124095_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:11:07.35 +46:55:58.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 1.492 977541157935274880 107.78121170371 +46.93278332141 13.8690 13.3615 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.492#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124098_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124098_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 124104_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124104_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:31:33.96 +41:26:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.630 958297226252177024 097.89207927200 +41.44442738742 12.9195 12.2446 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.630#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124106_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124106_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 124107_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124107_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:32:04.21 +41:12:09.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 1.730 957539112984773760 098.01691540233 +41.20254410685 13.1815 12.7301 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.730#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124110_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
Preparing report for the candidate 124110_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
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Considering the candidate 124115_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124115_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:51:51.98 +42:51:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 2.182 925604278792887296 117.96739174599 +42.85809986358 13.5555 12.9625 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.182#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124116_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124116_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:04:49.23 +47:06:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.113 977684609842934144 106.20596196662 +47.10116908714 13.5262 12.8468 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.113#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124129_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124129_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:31:08.97 +50:39:25.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 5.041 968199638427409920 097.78526666090 +50.65663781845 12.4929 11.7882 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124133_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
Preparing report for the candidate 124133_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
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Considering the candidate 124137_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124137_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:28:22.07 +45:20:44.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.20, MAG_FAINT_SEARCH_LIMIT=14.18)GAIADR2_OUTPUT=# 0.670 965338567436942848 097.09171549378 +45.34564787216 12.7332 12.2360 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124139_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124139_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:42:08.82 +49:24:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 0.829 981997066245835904 115.53699858919 +49.40064157456 13.2797 12.8029 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.829#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124140_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124140_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:26:49.96 +48:26:36.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 3.995 967554053303255552 096.70650945872 +48.44326433229 12.4577 11.7387 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124144_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124144_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 124146_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
Preparing report for the candidate 124146_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
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Considering the candidate 124148_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124148_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:27:57.26 +46:47:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 0.684 965855067319531776 096.98840642931 +46.79357571567 12.6138 12.1239 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.684#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124150_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124150_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:28:13.26 +47:01:10.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 1.203 965905365680600448 097.05556431394 +47.01927136837 12.6070 11.8806 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.203#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124152_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124152_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:47:45.57 +41:37:13.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.22, MAG_FAINT_SEARCH_LIMIT=14.20)
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Considering the candidate 124156_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
Preparing report for the candidate 124156_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
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Considering the candidate 124164_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124164_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:31:05.41 +41:38:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.04, MAG_FAINT_SEARCH_LIMIT=14.02)GAIADR2_OUTPUT=# 1.277 924721753209722496 112.77299451418 +41.63453284916 12.8945 12.3658 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.277#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124169_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124169_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:32:21.55 +50:41:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 4.858 992216885091626752 098.09186794299 +50.68625458480 12.1911 11.6611 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124178_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124178_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 124184_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124184_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:31:55.12 +42:37:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.02, MAG_FAINT_SEARCH_LIMIT=13.00)GAIADR2_OUTPUT=# 0.567 924879258249868032 112.97972034302 +42.61801360414 11.9326 11.5140 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124186_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124186_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:05:32.86 +51:01:39.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.91, MAG_FAINT_SEARCH_LIMIT=12.89)GAIADR2_OUTPUT=# 0.878 980825807189640448 106.38679757766 +51.02746238318 12.1690 11.3420 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.878#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124475_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124475_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:53:14.25 +41:05:18.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 2.269 951527327002437760 103.31006502238 +41.08819944193 12.9173 12.2670 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.269#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124489_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124489_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:00:36.97 +42:05:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.96, MAG_FAINT_SEARCH_LIMIT=13.94)GAIADR2_OUTPUT=# 1.092 951263104910749824 105.15435531597 +42.09766638302 12.8301 12.1299 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.092#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124572_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124572_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:03:40.52 +44:53:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.26, MAG_FAINT_SEARCH_LIMIT=14.24)GAIADR2_OUTPUT=# 1.911 953409970082188672 105.91957991996 +44.89187297678 13.2545 12.5511 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.911#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124587_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124587_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:31:43.72 +44:33:17.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.21, MAG_FAINT_SEARCH_LIMIT=14.19)GAIADR2_OUTPUT=# 0.663 973458121505945728 112.93240172759 +44.55475659674 12.9614 12.3770 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.663#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124620_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124620_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:03:26.14 +47:54:03.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 1.617 978584761972912384 105.85911318704 +47.90059838833 13.4904 12.9859 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.617#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124638_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124638_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:18:22.86 +41:05:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.40, MAG_FAINT_SEARCH_LIMIT=14.38)GAIADR2_OUTPUT=# 0.636 948513432487644672 109.59543879143 +41.09075649818 13.5671 13.0669 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.636#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124660_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124660_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:54:05.53 +40:53:49.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.38, MAG_FAINT_SEARCH_LIMIT=14.36)GAIADR2_OUTPUT=# 1.161 950770180103373568 103.52320392331 +40.89689615942 13.4694 13.0251 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124676_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124676_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:01:59.24 +44:25:17.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.43, MAG_FAINT_SEARCH_LIMIT=14.41)GAIADR2_OUTPUT=# 1.415 953042252162410880 105.49722174936 +44.42133267252 13.4284 13.0942 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.415#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124684_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124684_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:52:35.53 +47:42:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 0.640 954736565221546752 103.14810306177 +47.71452148868 13.6027 13.1875 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.640#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124721_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124721_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:57:43.45 +45:07:28.9 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 124768_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124768_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:14:05.23 +46:50:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 1.801 977851254574393216 108.52250167553 +46.84157384767 13.9683 13.3553 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.801#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124818_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124818_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:54:46.31 +41:34:49.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 1.631 951563374664068864 103.69302208466 +41.57991060789 13.7694 13.1262 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.631#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124819_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124819_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:57:31.14 +49:15:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 5.300 979271342561896064 104.38011041129 +49.25775876527 13.8835 13.4623 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124828_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124828_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 124835_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124835_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:55:04.82 +45:49:50.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 124836_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124836_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:26:51.10 +44:27:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 1.709 973265535172528000 111.71343618362 +44.45920363782 13.7533 13.2487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.709#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124864_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124864_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:42:08.12 +48:40:32.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.96, MAG_FAINT_SEARCH_LIMIT=14.94)GAIADR2_OUTPUT=# 1.445 967080056415533568 100.53431789887 +48.67602014201 13.8903 13.3505 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.445#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124932_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124932_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:14:42.94 +41:47:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 3.469 949359060008408960 108.67988475390 +41.78716707405 14.0768 13.5524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.469#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124938_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124938_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:54:47.77 +41:04:15.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.01, MAG_FAINT_SEARCH_LIMIT=14.99)GAIADR2_OUTPUT=# 2.375 950778804397687040 103.69984655109 +41.07071323950 14.2000 13.9080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.375#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124941_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124941_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:10:54.60 +49:54:11.3 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=14.15, MAG_FAINT_SEARCH_LIMIT=15.13)
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Considering the candidate 124942_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124942_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:45:28.96 +43:07:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 3.281 963947723882749568 101.37093480178 +43.13002651187 13.9399 13.3454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124947_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124947_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:52:59.89 +42:24:03.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)
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Considering the candidate 124949_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124949_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:51:34.50 +48:22:45.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 3.231 990800924569671040 102.89499197751 +48.37881339386 14.3830 13.9185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.231#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124983_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 124983_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:18:01.66 +48:16:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 0.403 976537956654734720 109.50678282476 +48.28118221212 14.3495 13.7938 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125011_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
Preparing report for the candidate 125011_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
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Considering the candidate 125041_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 125041_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:00:46.90 +47:57:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 2.756 978626960028656000 105.19510430279 +47.96604210471 14.4980 13.9297 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125079_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 125079_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:07:07.62 +41:56:35.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.22, MAG_FAINT_SEARCH_LIMIT=15.20)GAIADR2_OUTPUT=# 2.946 952513249630878592 106.78259524284 +41.94253157048 14.2939 13.8332 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.946#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125086_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 125086_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:09:48.57 +46:26:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 2.794 977498483140351104 107.45321267105 +46.43470336649 14.3801 13.8428 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125099_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 125099_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:27:29.99 +45:40:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 2.850 973840373595415936 111.87582034475 +45.67684712888 14.1472 13.5866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.850#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125108_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 125108_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:52:50.33 +42:24:03.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.07, MAG_FAINT_SEARCH_LIMIT=15.05)GAIADR2_OUTPUT=# 2.681 952024344913526912 103.20952287272 +42.40032354899 14.1325 13.6793 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125143_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 125143_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:04:00.70 +47:01:30.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 2.840 977694952124197888 106.00381529360 +47.02453090981 14.4394 13.8480 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125157_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 125157_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:12:28.95 +45:14:51.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 2.994 974288012267298944 108.12173188076 +45.24787365933 14.4875 13.9304 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.994#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125167_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 125167_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:45:32.36 +41:36:33.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 3.151 924121179341553152 116.38600376133 +41.60937360571 14.7602 14.2546 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.151#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118710_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 118710_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
Rejecting candidate due to large distance (25.4") between the two second-epoch detections
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Considering the candidate 102375_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 102375_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 06:41:13.10 +44:10:01.1 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 91832_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 91832_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
Rejecting candidate due to large distance (29.0") between the two second-epoch detections
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Considering the candidate 24471_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 24471_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:56:51.16 +47:45:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.20, MAG_FAINT_SEARCH_LIMIT=15.18)GAIADR2_OUTPUT=# 2.383 932787048955098368 119.21353274865 +47.75488544496 14.3009 13.7958 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.383#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 120773_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 120773_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
Rejecting candidate due to large distance (26.0") between the two second-epoch detections
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Considering the candidate 116292_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 116292_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:51:42.50 +49:23:04.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 2.582 934228577419145600 117.92601261014 +49.38438597385 13.3404 12.7713 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.582#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 116159_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 116159_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
**** FOUND 07:41:06.88 +50:15:35.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 4.112 982244765599819392 115.27869829594 +50.25874681905 13.8591 13.2516 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.112#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 36766_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 36766_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks
Rejecting candidate due to large distance (26.1") between the two second-epoch detections
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Considering the candidate 52210_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
Preparing report for the candidate 52210_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
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Considering the candidate 86737_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047
The candidate 86737_fd_Lyn-03-Q2b1x1_2026-03-19_02-47-34_20.00sec_-15.00C_LIGHT_0047 did not pass the final checks