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_230146_TTUQ2b1x1_18772_DKpgey8W
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 14.50 06:29:19.49 +48:32:59.2
166.35673 16.55990 galactic Aur Second-epoch detections are separated by 2.5" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:29:19.49 +48:32:59.2 (user input) | T | P | (position from user input) SpType: G2 (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,2461119.6596,14.50,0.05,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 20260320.1596 14.50CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:29:19.49 +48:32:59.2 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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,2461119.6596,14.34,0.05,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
target 20260320.1596 14.34CV 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/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:30:18.71 +50:34:03.2 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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,2461119.6596,14.36,0.05,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 20260320.1596 14.36CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:40.43 +47:21:13.4 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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,2461119.6596,14.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1596 14.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:35.13 +48:21:30.0 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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,2461119.6596,14.14,0.05,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 20260320.1596 14.14CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:30.12 +49:56:22.6 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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,2461119.6596,13.97,0.05,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 20260320.1596 13.97CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:36:17.88 +50:39:04.1 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 14.16 06:26:29.17 +49:04:09.3
165.66933 16.32834 galactic Aur Second-epoch detections are separated by 2.1" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:26:29.17 +49:04:09.3 (user input) | T | P | (position from user input) SpType: K4 (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,2461119.6596,14.16,0.05,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
target 20260320.1596 14.16CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:29.17 +49:04:09.3 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 14.19 06:30:32.00 +49:04:53.6
165.92160 16.94560 galactic Aur Second-epoch detections are separated by 2.2" 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 | ATO J097.6329+49.0831 | 06:30:32.00 +49:04:53.6 (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 J097.6329+49.0831,2461119.6596,14.19,0.05,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 J097.6329+49.0831 20260320.1596 14.19CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:30:32.00 +49:04:53.6 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 14.21 06:31:20.71 +50:09:43.5
164.92319 17.47025 galactic Aur Second-epoch detections are separated by 2.5" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:31:20.71 +50:09:43.5 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6596,14.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1596 14.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:20.71 +50:09:43.5 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 14.22 06:28:52.06 +50:31:19.1
164.41924 17.23701 galactic Aur Second-epoch detections are separated by 3.6" and 3.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:28:52.06 +50:31:19.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6596,14.22,0.05,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 20260320.1596 14.22CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:28:52.06 +50:31:19.1 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 14.15 06:26:50.66 +49:02:21.1
165.72188 16.37081 galactic Aur Second-epoch detections are separated by 4.7" 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 | 06:26:50.66 +49:02:21.1 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6596,14.15,0.05,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 20260320.1596 14.15CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:50.66 +49:02:21.1 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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,2461119.6596,14.06,0.05,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 20260320.1596 14.06CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:30:32.38 +49:37:46.5 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 14.03 06:27:32.07 +48:51:10.0
165.94672 16.40339 galactic Aur Second-epoch detections are separated by 0.8" 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 | target | 06:27:32.07 +48:51:10.0 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6596,14.03,0.05,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 20260320.1596 14.03CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:32.07 +48:51:10.0 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 14.10 06:25:09.87 +49:20:02.8
165.32768 16.23236 galactic Aur Second-epoch detections are separated by 0.3" and 4.2 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 | 06:25:09.87 +49:20:02.8 (user input) | T | P | (position from user input) SpType: F9 (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,2461119.6596,14.10,0.05,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 20260320.1596 14.10CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:09.87 +49:20:02.8 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 14.13 06:26:23.24 +49:11:35.7
165.54367 16.36146 galactic Aur Second-epoch detections are separated by 3.3" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:26:23.24 +49:11:35.7 (user input) | T | P | (position from user input) SpType: F5 (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,2461119.6596,14.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1596 14.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:23.24 +49:11:35.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 13.82 06:31:22.74 +50:08:11.7
164.95013 17.46588 galactic Aur Second-epoch detections are separated by 2.1" and 4.2 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 | 06:31:22.74 +50:08:11.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6596,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1596 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:22.74 +50:08:11.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 13.78 06:27:16.11 +48:54:33.0
165.87491 16.38479 galactic Aur Second-epoch detections are separated by 1.5" 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 | target | 06:27:16.11 +48:54:33.0 (user input) | T | P | (position from user input) SpType: G2 (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,2461119.6596,13.78,0.05,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 20260320.1596 13.78CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:16.11 +48:54:33.0 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 13.81 06:26:01.26 +49:32:47.3
165.18008 16.44312 galactic Aur Second-epoch detections are separated by 0.5" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:26:01.26 +49:32:47.3 (user input) | T | P | (position from user input) SpType: G8 (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,2461119.6596,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1596 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:01.26 +49:32:47.3 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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,2461119.6596,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1596 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:29:31.20 +50:34:58.9 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 13.66 06:30:54.22 +50:40:59.0
164.38808 17.59677 galactic Aur Second-epoch detections are separated by 1.4" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:30:54.22 +50:40:59.0 (user input) | T | P | (position from user input) SpType: F9 (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,2461119.6596,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1596 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:30:54.22 +50:40:59.0 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 13.64 06:26:49.18 +48:51:59.4
165.88618 16.30025 galactic Aur Second-epoch detections are separated by 0.6" and 4.2 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 | 06:26:49.18 +48:51:59.4 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6596,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1596 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:49.18 +48:51:59.4 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 13.72 06:25:08.96 +49:08:26.6
165.51208 16.15459 galactic Aur Second-epoch detections are separated by 3.8" and 4.8 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 | 06:25:08.96 +49:08:26.6 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6596,13.72,0.05,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 20260320.1596 13.72CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:08.96 +49:08:26.6 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 13.50 06:28:02.54 +50:32:59.6
164.34064 17.12593 galactic Aur Second-epoch detections are separated by 2.5" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:28:02.54 +50:32:59.6 (user input) | T | P | (position from user input) SpType: F9 (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,2461119.6596,13.50,0.05,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 20260320.1596 13.50CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:28:02.54 +50:32:59.6 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 13.49 06:31:01.21 +50:28:48.7
164.59307 17.53930 galactic Aur Second-epoch detections are separated by 2.3" and 4.0 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 | 06:31:01.21 +50:28:48.7 (user input) | T | P | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6596,13.49,0.05,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
target 20260320.1596 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:01.21 +50:28:48.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 13.51 06:28:20.85 +49:53:35.5
164.99587 16.92320 galactic Aur Second-epoch detections are separated by 2.4" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 968092088149937280 | 06:28:21.55 +49:53:36.2 (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 968092088149937280,2461119.6596,13.51,0.05,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 968092088149937280 20260320.1596 13.51CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:28:20.85 +49:53:35.5 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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,2461119.6596,13.62,0.05,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
target 20260320.1596 13.62CV 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/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:56.05 +48:21:08.6 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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,2461119.6596,13.48,0.05,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 20260320.1596 13.48CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:10.52 +47:02:32.2 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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,2461119.6596,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1596 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:35.07 +50:34:33.6 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 13.45 06:30:22.92 +49:10:00.1
165.82940 16.95470 galactic Aur Second-epoch detections are separated by 1.3" 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 967638573962507392 | 06:30:23.60 +49:10:01.2 (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 967638573962507392,2461119.6596,13.45,0.05,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 967638573962507392 20260320.1596 13.45CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:30:22.92 +49:10:00.1 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 13.38 06:31:07.47 +50:39:24.7
164.42713 17.61969 galactic Aur Second-epoch detections are separated by 3.9" 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 968199638427409920 | 06:31:08.46 +50:39:23.9 (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 968199638427409920,2461119.6596,13.38,0.05,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 968199638427409920 20260320.1596 13.38CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:07.47 +50:39:24.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 13.27 06:26:30.67 +50:02:42.8
164.73155 16.70807 galactic Aur Second-epoch detections are separated by 1.3" and 4.0 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 J096.6219+50.0420 | 06:26:29.33 +50:02:45.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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
ATO J096.6219+50.0420,2461119.6596,13.27,0.05,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 J096.6219+50.0420 20260320.1596 13.27CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:30.67 +50:02:42.8 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 13.37 06:28:08.99 +49:21:05.5
165.50652 16.68770 galactic Aur Second-epoch detections are separated by 1.2" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 967690594607539968 | 06:28:09.67 +49:21:07.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 967690594607539968,2461119.6596,13.37,0.05,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 967690594607539968 20260320.1596 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:28:08.99 +49:21:05.5 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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,2461119.6596,13.35,0.05,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 20260320.1596 13.35CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:52.65 +49:39:06.5 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 13.11 06:25:09.53 +49:52:38.3
164.80578 16.44267 galactic Aur Second-epoch detections are separated by 2.1" and 4.0 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 970719165026273152 | 06:25:08.31 +49:52:39.5 (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 970719165026273152,2461119.6596,13.11,0.05,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 970719165026273152 20260320.1596 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:09.53 +49:52:38.3 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 12.85 06:29:04.45 +49:48:46.3
165.11990 17.00130 galactic Aur Second-epoch detections are separated by 1.1" and 4.0 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 968078997090049024 | 06:29:03.64 +49:48:45.9 (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 968078997090049024,2461119.6596,12.85,0.05,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 968078997090049024 20260320.1596 12.85CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:29:04.45 +49:48:46.3 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 12.96 06:27:26.70 +50:32:51.2
164.30544 17.03717 galactic Aur Second-epoch detections are separated by 2.1" and 3.8 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 968227431158742400 | 06:27:27.61 +50:32:51.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 968227431158742400,2461119.6596,12.96,0.05,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 968227431158742400 20260320.1596 12.96CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:26.70 +50:32:51.2 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 12.56 06:31:08.43 +50:06:11.0
164.96799 17.41797 galactic Aur Second-epoch detections are separated by 0.4" and 4.2 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 968154451074666624 | 06:31:09.23 +50:06:10.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 968154451074666624,2461119.6596,12.56,0.05,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 968154451074666624 20260320.1596 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:08.43 +50:06:11.0 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 12.50 06:27:38.01 +48:53:33.2
165.91500 16.43374 galactic Aur Second-epoch detections are separated by 1.0" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 967661010873110272 | 06:27:38.62 +48:53:35.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 967661010873110272,2461119.6596,12.50,0.05,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 967661010873110272 20260320.1596 12.50CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:27:38.01 +48:53:33.2 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 11.74 06:26:22.04 +47:49:03.4
166.86061 15.82172 galactic Aur Second-epoch detections are separated by 2.5" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 966008861508539392 | 06:26:23.01 +47:49:05.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K1 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 966008861508539392,2461119.6596,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 966008861508539392 20260320.1596 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:22.04 +47:49:03.4 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 11.66 06:26:36.61 +48:19:43.3
166.38808 16.05922 galactic Aur Second-epoch detections are separated by 0.9" and 4.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 967531371579143168 | 06:26:37.65 +48:19:44.0 (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 967531371579143168,2461119.6596,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 967531371579143168 20260320.1596 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:36.61 +48:19:43.3 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 11.04 06:26:11.82 +50:26:18.0
164.33216 16.81207 galactic Aur Second-epoch detections are separated by 1.0" and 4.2 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 J096.5497+50.4299 | 06:26:10.58 +50:26:21.7 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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
ATO J096.5497+50.4299,2461119.6596,11.04,0.05,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 J096.5497+50.4299 20260320.1596 11.04CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:11.82 +50:26:18.0 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 10.19 06:26:03.74 +48:05:03.9
166.58471 15.87959 galactic Aur Second-epoch detections are separated by 6.1" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J096.5270+48.0745 | 06:26:04.35 +48:05:04.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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
ATO J096.5270+48.0745,2461119.6596,10.19,0.05,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 J096.5270+48.0745 20260320.1596 10.19CV 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:26:03.74 +48:05:03.9 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1596 2461119.6596 12.94 07:59:05.11 +49:55:14.6
168.89787 31.03677 galactic Lyn Second-epoch detections are separated by 0.8" and 3.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:59:05.11 +49:55:14.6 (user input) | T | P | (position from user input) J-Ks=0.262+/-0.028 (F)
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,2461119.6596,12.94,0.05,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 20260320.1596 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:59:05.11 +49:55:14.6 ;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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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_22-50-01_20_00sec_-15_00C_LIGHT_0121_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_22-49-15_20_00sec_-14_90C_LIGHT_0120_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: 2461119.65985791 20.03.2026 03:50:01.723 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 22
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: 7 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 18704
Objects passed selection criteria: 18699
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 17924
Average stars matched: 17373.8 (96.9301 %)
Memory usage VmPeak: 122480 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 23:05:50 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: 2461119.65985791 20.03.2026 03:50:01.723 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 699
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: 61 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): 106037
Objects passed selection criteria: 105797
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 100498
Average stars matched: 96718.5 (96.2392 %)
Memory usage VmPeak: 1889512 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 23:08:05 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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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: 2461119.65932591
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_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits exists and is non-empty
Saving wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits to local_wcs_cache/
'wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits' -> 'local_wcs_cache/wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits'
wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits exists and is non-empty
Saving wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits to local_wcs_cache/
'wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits' -> 'local_wcs_cache/wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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 07:11:53.147 +45:59:29.80
Angular distance between the image centers 0.02 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 07:11:52.504 +45:59:52.51
Angular distance between the image centers 0.02 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 07:11:53.147 +45:59:29.80
Second-epoch second image center 07:11:52.504 +45:59:52.51
Angular distance between the image centers 0.00658 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.z7ZSHebvFO
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.G85RvAlrCc
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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits &> /tmp/tmp.8Ich35iEJU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits &> /tmp/tmp.ahSTtM1aiw
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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 22 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_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
2.5 pix fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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
15.4 mag. fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
15.4 mag. fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 12.5 (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.z7ZSHebvFO (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_230146_TTUQ2b1x1_18772_DKpgey8W/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.G85RvAlrCc (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_230146_TTUQ2b1x1_18772_DKpgey8W/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.8Ich35iEJU (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_230146_TTUQ2b1x1_18772_DKpgey8W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
WCS-calibrated image found: wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
Checking if the catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits.cat corresponding to the image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits.cat corresponding to the image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.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_22-49-15_20.00sec_-14.90C_LIGHT_0120.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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
WCS catalog name: wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1234, passed=18052
Got 18052 stars (including 16802 good ones) from the SExtractor catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits.cat
util/solve_plate_with_UCAC5 got 18052 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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: 0.69"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.67"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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: 0.68"
Estimated accuracy of the plate solution: 0.73"
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_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits -region wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.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.ahSTtM1aiw (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_230146_TTUQ2b1x1_18772_DKpgey8W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
WCS-calibrated image found: wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
Checking if the catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits.cat corresponding to the image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits.cat corresponding to the image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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_22-50-01_20.00sec_-15.00C_LIGHT_0121.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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
WCS catalog name: wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1228, passed=18081
Got 18081 stars (including 16836 good ones) from the SExtractor catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits.cat
util/solve_plate_with_UCAC5 got 18081 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.65"
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: 0.65"
Estimated accuracy of the plate solution: 0.69"
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_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits -region wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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_230146_TTUQ2b1x1_18772_DKpgey8W/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_230146_TTUQ2b1x1_18772_DKpgey8W/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_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits'
Saving fully-calibrated image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits'
Preparing the HTML report for the field Lyn-03-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20968.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20970.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out20971.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21149.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21166.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21170.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21173.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21189.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21193.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21195.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21196.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21200.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21203.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21212.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21213.dat to exclusion_list_gaiadr2.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
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Considering the candidate 20968_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 20968_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:25:08.80 +50:04:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.57, MAG_FAINT_SEARCH_LIMIT=12.55)GAIADR2_OUTPUT=# 5.501 971109152352791040 096.28428550082 +50.08145970170 10.9361 10.2454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.501#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20969_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 20969_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:58:43.66 +47:38:57.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20970_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 20970_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:27:00.15 +50:22:46.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.52, MAG_FAINT_SEARCH_LIMIT=12.50)GAIADR2_OUTPUT=# 5.453 971133341608535936 096.75300036455 +50.37969615523 10.7071 10.0302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20971_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 20971_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:27:49.88 +49:22:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 5.080 967702590451955072 096.95993961605 +49.37469338151 10.3504 9.6832 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.080#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21046_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21046_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:21:09.55 +45:48:14.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21122_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21122_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:29:46.29 +49:40:28.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 21132_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21132_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:14:00.44 +46:50:13.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.787 977851288934133376 108.50169777119 +46.83674646194 12.2566 11.7036 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.787#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21146_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21146_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:39:57.78 +44:02:24.2 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 21149_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21149_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:22:12.39 +50:54:47.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.681 980272001222749056 110.55178610777 +50.91324289648 12.3837 11.9421 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.681#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21166_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21166_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:23:03.28 +47:26:17.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.666 976247513786488832 110.76359356562 +47.43804395155 12.2823 11.7143 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21170_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21170_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:45:24.26 +47:36:24.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.522 966685988872955776 101.35162865376 +47.60670813433 12.4778 11.9812 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21173_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21173_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:41:18.36 +44:36:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.058 964626633657667584 100.32678694075 +44.60109421225 12.4334 11.9479 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.058#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21186_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21186_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:09:44.08 +49:20:29.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 0.773 979838072087546368 107.43399305478 +49.34141403288 12.5382 12.1238 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.773#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21189_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21189_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:19:37.22 +45:52:28.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 0.866 974562306059394816 109.90534652158 +45.87428850370 12.2462 11.5093 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.866#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21193_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21193_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:18:59.87 +50:29:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.56, MAG_FAINT_SEARCH_LIMIT=13.54)GAIADR2_OUTPUT=# 1.021 980152291894006912 109.74974784218 +50.48595093202 12.4695 12.0512 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.021#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21195_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21195_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:09:17.97 +46:36:36.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.59, MAG_FAINT_SEARCH_LIMIT=13.57)GAIADR2_OUTPUT=# 0.897 977513975086332800 107.32518021542 +46.60997628456 12.2982 11.5787 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.897#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21196_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21196_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:14:14.57 +42:35:42.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.57, MAG_FAINT_SEARCH_LIMIT=13.55)GAIADR2_OUTPUT=# 0.315 949602700616545408 108.56082511403 +42.59518346042 12.2986 11.6357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.315#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21200_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21200_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:07:42.60 +49:13:44.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.61, MAG_FAINT_SEARCH_LIMIT=13.59)GAIADR2_OUTPUT=# 1.346 978379943572439040 106.92787114238 +49.22882626694 12.5718 12.2606 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.346#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 21203_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21203_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:25:07.11 +47:22:27.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 0.559 976237373367232384 111.27970438348 +47.37413209335 12.4958 12.0357 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.559#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21212_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21212_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:30:27.30 +48:16:55.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 1.026 975970265057352448 112.61391293451 +48.28170868704 12.3604 11.7077 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.026#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21213_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21213_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:41:08.10 +49:56:49.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.58, MAG_FAINT_SEARCH_LIMIT=13.56)GAIADR2_OUTPUT=# 1.071 982029123881601280 115.28421091507 +49.94694889180 12.4245 11.8423 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.071#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 11459_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 11459_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:41:13.16 +44:10:01.4 in the exclusion list exclusion_list.txt ****
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 ####
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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits exists and is non-empty
wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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 07:11:53.147 +45:59:29.80
Angular distance between the image centers 0.02 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 07:11:52.504 +45:59:52.51
Angular distance between the image centers 0.02 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 07:11:53.147 +45:59:29.80
Second-epoch second image center 07:11:52.504 +45:59:52.51
Angular distance between the image centers 0.00658 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.8hm3gAc2ub
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.4dnlYqfoIw
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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits &> /tmp/tmp.Zstez1gM5L
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits &> /tmp/tmp.Dr8ALoPrgL
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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 302 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
2.3 pix fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
2.4 pix fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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
15.5 mag. fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
15.5 mag. fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
All-image limiting magnitude estimate: 15.5 (SNR ) 14.8 (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.8hm3gAc2ub (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_230146_TTUQ2b1x1_18772_DKpgey8W/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
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
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.4dnlYqfoIw (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_230146_TTUQ2b1x1_18772_DKpgey8W/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.Zstez1gM5L (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_230146_TTUQ2b1x1_18772_DKpgey8W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
WCS-calibrated image found: wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
Checking if the catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits.cat corresponding to the image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits.cat corresponding to the image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.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_22-49-15_20.00sec_-14.90C_LIGHT_0120.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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
WCS catalog name: wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=8369, passed=96530
Got 96530 stars (including 88058 good ones) from the SExtractor catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits.cat
util/solve_plate_with_UCAC5 got 96530 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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: 0.64"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.60"
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: 0.60"
Estimated accuracy of the plate solution: 0.66"
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_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits -region wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.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.Dr8ALoPrgL (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_230146_TTUQ2b1x1_18772_DKpgey8W/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-03-Q2b1x1_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
WCS-calibrated image found: wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
Checking if the catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits.cat corresponding to the image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits.cat corresponding to the image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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_22-50-01_20.00sec_-15.00C_LIGHT_0121.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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
WCS catalog name: wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=8333, passed=96450
Got 96450 stars (including 88011 good ones) from the SExtractor catalog wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits.cat
util/solve_plate_with_UCAC5 got 96450 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.1'
Seting catalog search parameters based on the expected field of view 937.1 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013015 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010412 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
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: 0.67"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
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: 0.62"
Estimated accuracy of the plate solution: 0.66"
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_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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_230146_TTUQ2b1x1_18772_DKpgey8W/fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits -region wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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_230146_TTUQ2b1x1_18772_DKpgey8W/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_230146_TTUQ2b1x1_18772_DKpgey8W/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_22-49-15_20.00sec_-14.90C_LIGHT_0120.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_230146_TTUQ2b1x1_18772_DKpgey8W/wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-49-15_20.00sec_-14.90C_LIGHT_0120.fits
Saving fully-calibrated image wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.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_230146_TTUQ2b1x1_18772_DKpgey8W/wcs_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121.fits
Preparing the HTML report for the field Lyn-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Adding exclusion_list_gaiadr2.txt__out124183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124186.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124189.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124201.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124221.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124228.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124229.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124230.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124232.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124240.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124247.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124257.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124258.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124260.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124263.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124267.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124271.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124276.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124280.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124290.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124297.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124301.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124309.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124313.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124320.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124324.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124330.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124332.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124339.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124346.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124354.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124360.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124363.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124371.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124374.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124376.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124380.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124382.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124386.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124390.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124396.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124406.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124407.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124410.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124414.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124421.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124427.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124445.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124449.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124450.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124454.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124458.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124469.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124472.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124476.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124480.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124490.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124505.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124510.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124512.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124768.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124799.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124831.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124868.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out124881.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125109.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125136.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125308.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125323.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125369.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125431.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125481.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125567.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out125604.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out98184.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out124350.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out03686.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124274.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124294.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124310.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124319.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124368.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124370.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124400.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124403.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124420.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124425.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124441.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124451.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124456.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124460.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124464.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124468.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124474.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124482.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124483.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124493.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124495.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124506.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124509.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out124511.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 85s
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: 27s
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Considering the candidate 124178_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124178_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
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Considering the candidate 124183_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124183_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:29:58.36 +49:05:40.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 3.596 967637440091142144 097.49466125714 +49.09446613355 13.7608 13.1569 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.596#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_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124186_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:29:34.78 +47:57:20.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 2.111 967462484600377600 097.39571498442 +47.95553672383 13.7725 13.2883 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.111#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124189_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124189_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:31:45.37 +41:21:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 4.523 958292179667443328 097.93782755422 +41.36363492144 13.7958 13.0385 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124201_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124201_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:35:54.61 +49:14:53.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 0.858 967826388588811520 098.97718352531 +49.24800981236 14.0311 13.4923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.858#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124211_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124211_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:37:47.91 +50:37:21.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 2.212 982317092849108096 114.44983777977 +50.62195613888 14.3893 13.8645 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124217_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124217_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124221_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124221_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:28:58.02 +47:03:03.6 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)
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Considering the candidate 124228_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124228_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:59:32.90 +49:46:57.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.39, MAG_FAINT_SEARCH_LIMIT=15.37)GAIADR2_OUTPUT=# 0.175 935624201272113792 119.88715864675 +49.78252614259 14.2464 13.8345 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.175#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124229_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124229_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:29:35.18 +50:01:05.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 3.727 968108344602530048 097.39819434435 +50.01810321281 13.5993 13.0408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.727#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124230_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124230_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:46:29.66 +46:51:22.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.43, MAG_FAINT_SEARCH_LIMIT=15.41)GAIADR2_OUTPUT=# 3.363 966277726461801728 101.62492984484 +46.85598179600 14.1377 13.6444 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.363#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124232_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124232_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:32:17.58 +42:13:24.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 3.098 958724493895976960 098.07440072943 +42.22367597226 13.8657 13.3293 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.098#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124234_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124234_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:40:34.38 +42:17:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 0.522 957851928339142016 100.14328455467 +42.29741271184 14.1080 13.4095 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124235_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124235_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:34:14.70 +49:50:07.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 1.539 967953004225148160 098.56080869956 +49.83498665939 13.8061 13.2696 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.539#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124240_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124240_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:27:16.27 +49:26:43.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 4.637 967706713620563072 096.81975995960 +49.44521524944 13.7052 13.1579 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.637#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124247_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124247_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:30:49.31 +50:34:26.0 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)
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Considering the candidate 124256_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124256_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:58:40.79 +50:15:43.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 0.454 935654089948166784 119.67004343529 +50.26219699218 14.1423 13.6528 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.454#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124257_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124257_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:30:21.69 +42:21:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.30, MAG_FAINT_SEARCH_LIMIT=15.28)GAIADR2_OUTPUT=# 1.051 972814632327073920 112.59074308247 +42.35192153586 14.0601 13.4744 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.051#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124258_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124258_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:29:35.29 +48:51:20.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 1.760 967605146234036864 097.39730768171 +48.85515452063 13.9553 13.4590 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.760#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124260_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124260_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:46:27.87 +46:00:09.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 0.763 966089057137990400 101.61633360309 +46.00234522722 14.4548 13.9489 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.763#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124262_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124262_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124263_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124263_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:27:33.43 +48:57:29.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.19, MAG_FAINT_SEARCH_LIMIT=15.17)GAIADR2_OUTPUT=# 1.247 967667268641047808 096.88944277667 +48.95780693665 13.4746 12.7573 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.247#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124265_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124265_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124267_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124267_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:27:43.64 +49:27:30.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 5.567 967703999201224192 096.92951993210 +49.45819466373 13.4077 12.7592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.567#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124270_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124270_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:27:28.43 +47:03:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 0.698 965953198732616320 096.86874204796 +47.06578928190 13.4374 12.7121 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.698#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124271_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124271_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:39:57.10 +42:53:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 1.024 964061111019686144 099.98811423586 +42.88769967764 14.3704 13.8989 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.024#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124274_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124274_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124276_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124276_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:32:11.09 +50:16:13.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.41, MAG_FAINT_SEARCH_LIMIT=15.39)GAIADR2_OUTPUT=# 1.756 968150744519728128 098.04561951658 +50.27010616299 13.6385 13.1554 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.756#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124280_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124280_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:54:14.90 +46:48:55.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.27, MAG_FAINT_SEARCH_LIMIT=15.25)GAIADR2_OUTPUT=# 1.912 954640323594653696 103.56272423693 +46.81506183018 14.2596 13.7866 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.912#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124288_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124288_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:58:29.04 +49:35:56.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124290_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124290_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:29:02.10 +44:33:37.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 3.577 965188518458449536 097.25788107719 +44.55963938069 13.7073 13.1156 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.577#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124291_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124291_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:37:36.57 +41:06:56.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124294_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124294_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124297_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124297_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:59:08.74 +49:55:26.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 0.827 935628771117303040 119.78668470432 +49.92398714588 13.9493 13.4541 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.827#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124299_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124299_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 124301_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124301_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:56:55.23 +47:38:27.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 2.521 978698119046831872 104.23107020998 +47.64068125107 14.1679 13.8650 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.521#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124302_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124302_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 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 124304_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124304_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:26:35.20 +49:52:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.32, MAG_FAINT_SEARCH_LIMIT=15.30)GAIADR2_OUTPUT=# 5.303 971091491447313664 096.64895062565 +49.88171293049 13.4045 12.8287 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.303#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124305_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124305_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124306_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124306_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124309_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124309_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:53:37.00 +41:07:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 2.172 951527125140205184 103.40470213369 +41.11802346577 14.3012 13.8167 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.172#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124310_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124310_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124312_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124312_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124313_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124313_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:47:02.74 +41:58:43.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 2.121 951777298394591872 101.76219204685 +41.97892803159 14.1344 13.5957 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.121#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124315_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124315_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 124316_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124316_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124319_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124319_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124320_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124320_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:29:30.77 +47:56:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 3.522 967460972771892352 097.37938865855 +47.94238184378 13.5028 12.7923 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124324_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124324_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:27:03.81 +50:30:07.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.02, MAG_FAINT_SEARCH_LIMIT=15.00)GAIADR2_OUTPUT=# 4.665 971229480156187648 096.76791214052 +50.50218114450 13.3820 12.8857 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.665#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124325_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124325_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 124330_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124330_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:26:02.31 +49:10:14.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.97, MAG_FAINT_SEARCH_LIMIT=14.95)GAIADR2_OUTPUT=# 4.467 970675566814750080 096.51147040806 +49.17103912383 13.3408 12.8087 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.467#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124332_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124332_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:33:05.17 +50:39:27.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 4.738 992204313724019968 098.27156960273 +50.65640619086 13.4093 12.8802 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.738#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124339_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124339_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:26:30.44 +47:35:15.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 1.010 965982026552902144 096.62644130172 +47.58762134709 13.3231 12.5398 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.010#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124341_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124341_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124346_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124346_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:30:17.13 +43:03:24.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 4.351 958824132840314240 097.56997089828 +43.05619446997 13.7223 13.2132 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.351#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124350_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124350_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:29:17.42 +50:18:03.1 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=13.89, MAG_FAINT_SEARCH_LIMIT=14.87)
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Considering the candidate 124354_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124354_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:31:25.00 +49:11:18.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 2.592 967998938898595328 097.85311894263 +49.18819377388 13.5510 13.0607 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.592#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124357_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124357_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:34:47.69 +49:07:17.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 2.741 967822231060501632 098.69979042608 +49.12172370250 13.4021 12.7571 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.741#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124360_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124360_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:45:08.16 +41:23:30.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 1.528 945735104042790528 101.28413425386 +41.39142100070 13.9037 13.3766 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.528#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124362_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124362_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124363_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124363_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:14:55.41 +40:56:46.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.93, MAG_FAINT_SEARCH_LIMIT=14.91)GAIADR2_OUTPUT=# 1.089 949182038636732672 108.73122074296 +40.94645849592 13.7343 13.2333 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124367_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124367_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124368_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124368_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124370_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124370_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124371_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124371_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:53:41.59 +50:24:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.84, MAG_FAINT_SEARCH_LIMIT=14.82)GAIADR2_OUTPUT=# 1.553 934399482757370112 118.42380087514 +50.40160458162 13.7114 13.2142 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124374_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124374_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:34:53.58 +49:50:04.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 3.876 967950938344462592 098.72488521042 +49.83488368306 13.2974 12.7789 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.876#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124376_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124376_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:36:46.31 +50:45:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.77, MAG_FAINT_SEARCH_LIMIT=14.75)GAIADR2_OUTPUT=# 1.814 992027700372291328 099.19259521318 +50.75357934072 13.2588 12.6805 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124380_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124380_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:30:36.35 +49:16:53.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.60, MAG_FAINT_SEARCH_LIMIT=14.58)GAIADR2_OUTPUT=# 4.780 968012171695019392 097.65304976334 +49.28224435151 13.0178 12.2920 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.780#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124382_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124382_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:58:02.36 +47:55:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.73, MAG_FAINT_SEARCH_LIMIT=14.71)GAIADR2_OUTPUT=# 2.633 933162635255063680 119.51092174613 +47.92872115131 13.2867 12.4033 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.633#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124383_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124383_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 124385_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124385_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 124386_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124386_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:29:38.58 +48:35:47.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.78, MAG_FAINT_SEARCH_LIMIT=14.76)GAIADR2_OUTPUT=# 1.532 967594803952952576 097.41122876858 +48.59621549107 13.3647 12.8134 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.532#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124390_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124390_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:27:21.58 +50:38:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 2.588 968229767620956672 096.84100243732 +50.63381714124 12.6938 11.9022 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124396_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124396_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:24:01.14 +50:31:15.3 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)
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Considering the candidate 124398_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124398_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:04:49.26 +47:06:05.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124399_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124399_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124400_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124400_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124403_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124403_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124405_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124405_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 124406_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124406_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:25:10.74 +49:49:12.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.76, MAG_FAINT_SEARCH_LIMIT=14.74)GAIADR2_OUTPUT=# 3.549 970718550847283456 096.29621789861 +49.81989285285 12.9736 12.2630 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.549#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124407_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124407_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:56:18.74 +43:58:15.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 2.319 953668458394155776 104.07897816143 +43.97084568718 13.6114 13.0317 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.319#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124409_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124409_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:26:15.10 +50:29:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.55, MAG_FAINT_SEARCH_LIMIT=14.53)GAIADR2_OUTPUT=# 3.490 971139251483540096 096.56442719858 +50.48818194936 12.6363 11.8863 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.490#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124410_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124410_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:29:07.94 +50:04:10.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 2.268 968111643137298304 097.28395715954 +50.06978706438 13.0459 12.5450 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.268#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124413_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124413_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 124414_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124414_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:32:16.77 +50:15:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.49, MAG_FAINT_SEARCH_LIMIT=14.47)GAIADR2_OUTPUT=# 3.661 968150671503442560 098.06829421524 +50.25583415487 12.8971 12.2208 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.661#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124415_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124415_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 124420_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124420_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124421_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124421_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:25:54.50 +48:38:26.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.65, MAG_FAINT_SEARCH_LIMIT=14.63)GAIADR2_OUTPUT=# 5.607 970561629922276864 096.47943332325 +48.64073292604 12.8558 12.1733 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.607#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124425_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124425_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124427_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124427_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:48:33.16 +42:10:08.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.62, MAG_FAINT_SEARCH_LIMIT=14.60)GAIADR2_OUTPUT=# 0.632 951830001937087232 102.13817382694 +42.16914773958 13.6482 13.1852 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.632#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124429_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124429_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 124430_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124430_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 124431_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124431_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124434_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124434_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124438_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124438_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:25:53.13 +50:26:36.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124439_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124439_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124441_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124441_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124442_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124442_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124445_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124445_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:24:55.39 +49:51:03.1 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.42, MAG_FAINT_SEARCH_LIMIT=14.40)
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Considering the candidate 124446_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124446_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124449_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124449_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:00:28.79 +46:03:31.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.35, MAG_FAINT_SEARCH_LIMIT=14.33)GAIADR2_OUTPUT=# 2.009 954348128378654848 105.12074841464 +46.05853543578 13.5210 13.0459 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.009#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124450_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124450_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:25:04.34 +49:37:05.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.52, MAG_FAINT_SEARCH_LIMIT=14.50)GAIADR2_OUTPUT=# 4.995 970709754754291200 096.27021896303 +49.61824139564 12.6092 12.0415 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.995#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124451_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124451_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124454_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124454_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:50:11.12 +50:33:33.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 0.901 934453427546578944 117.54656831808 +50.55899358479 13.1687 12.6185 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.901#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124456_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124456_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124458_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124458_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:32:02.71 +50:22:57.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.08, MAG_FAINT_SEARCH_LIMIT=14.06)GAIADR2_OUTPUT=# 3.809 968186714868988032 098.01291483984 +50.38280300461 12.4465 11.7926 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.809#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124460_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124460_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124462_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124462_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 124464_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124464_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124465_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124465_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124468_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124468_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124469_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124469_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:03:06.27 +41:36:33.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.17, MAG_FAINT_SEARCH_LIMIT=14.15)GAIADR2_OUTPUT=# 1.076 951038632739073280 105.77637840970 +41.60918553284 12.9909 12.3638 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.076#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124472_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124472_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:27:09.05 +48:35:33.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.23, MAG_FAINT_SEARCH_LIMIT=14.21)GAIADR2_OUTPUT=# 5.574 967562535861838848 096.78999299955 +48.59289275457 12.2969 11.5352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.574#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124474_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124474_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124476_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124476_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:25:41.38 +50:22:27.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.24, MAG_FAINT_SEARCH_LIMIT=14.22)GAIADR2_OUTPUT=# 4.888 971131761060597888 096.42454002651 +50.37429148710 12.1887 11.4728 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.888#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124478_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124478_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:31:05.46 +41:38:04.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124480_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124480_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:27:14.98 +50:07:11.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 5.695 968121671884668032 096.81488408858 +50.11980180876 12.1645 11.4530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.695#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124482_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124482_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124483_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124483_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124490_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124490_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:25:40.88 +49:59:57.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 4.792 971096198731476352 096.42231345242 +49.99980619286 11.7879 11.0895 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.792#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124493_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124493_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124495_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124495_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124503_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124503_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 124504_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124504_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124505_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124505_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:27:00.33 +50:22:46.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.56, MAG_FAINT_SEARCH_LIMIT=12.54)GAIADR2_OUTPUT=# 3.817 971133341608535936 096.75300036455 +50.37969615523 10.7071 10.0302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.817#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124506_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124506_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124509_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124509_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124510_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124510_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:01:10.69 +41:41:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.45, MAG_FAINT_SEARCH_LIMIT=11.43)GAIADR2_OUTPUT=# 0.557 951148446463574016 105.29464103713 +41.68808035943 10.4102 9.9433 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.557#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124511_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 124511_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
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Considering the candidate 124512_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124512_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:26:17.45 +50:24:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.21, MAG_FAINT_SEARCH_LIMIT=11.19)GAIADR2_OUTPUT=# 3.614 971134230664841344 096.57396364320 +50.40663414381 9.2116 8.4562 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.614#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124596_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124596_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 124605_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124605_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 124639_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124639_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 124643_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124643_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 124677_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124677_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
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Considering the candidate 124701_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124701_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 124719_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124719_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 124723_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124723_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 124739_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124739_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 124741_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124741_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
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Considering the candidate 124750_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124750_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 124752_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124752_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
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Considering the candidate 124755_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124755_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 124768_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124768_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:37:44.03 +45:09:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.84, MAG_FAINT_SEARCH_LIMIT=13.82)GAIADR2_OUTPUT=# 0.418 964702572975660032 099.43353298970 +45.16160334549 12.8397 12.4822 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.418#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124770_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124770_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 124772_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124772_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 124773_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124773_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 124778_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124778_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 124781_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124781_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 124784_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124784_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
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Considering the candidate 124786_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124786_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 124789_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124789_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 124791_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124791_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:53:14.24 +41:05:17.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124799_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124799_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:41:49.97 +46:04:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.92, MAG_FAINT_SEARCH_LIMIT=13.90)GAIADR2_OUTPUT=# 3.449 966310711810702208 100.45954802550 +46.07757304539 12.8425 12.3372 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.449#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124809_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124809_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 124814_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124814_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 124827_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124827_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 124831_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124831_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:36:52.27 +44:44:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.10, MAG_FAINT_SEARCH_LIMIT=14.08)GAIADR2_OUTPUT=# 0.455 964326265120851840 099.21793475583 +44.73623051475 12.9633 12.3530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.455#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124833_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124833_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (24.2") between the two second-epoch detections
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Considering the candidate 124840_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124840_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 124842_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124842_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 124843_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124843_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 124852_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124852_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 124864_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124864_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 124868_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124868_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:49:48.31 +41:30:04.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 1.588 951516404902135168 102.45176801097 +41.50093496735 13.1980 12.7487 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.588#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124876_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124876_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
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Considering the candidate 124878_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124878_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 124881_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124881_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:43:09.79 +45:38:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.07, MAG_FAINT_SEARCH_LIMIT=14.05)GAIADR2_OUTPUT=# 2.196 964612756619200640 100.79165217126 +45.64365656382 12.7328 12.2751 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.196#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 124885_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124885_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
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Considering the candidate 124886_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124886_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124887_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124887_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:31:43.71 +44:33:17.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124890_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124890_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124891_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124891_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 124920_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124920_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124924_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124924_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 124931_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124931_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 124932_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124932_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124937_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124937_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 124953_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124953_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:01:59.21 +44:25:17.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 124964_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124964_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 124967_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124967_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 124968_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124968_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 124969_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124969_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 124978_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124978_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 124986_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124986_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 124989_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124989_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 124998_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124998_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 124999_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 124999_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125003_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125003_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125011_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125011_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:52:35.55 +47:42:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125014_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125014_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:12:56.07 +41:58:44.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.358 949559136764508160 108.23487575474 +41.97906314824 13.7526 13.3071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.358#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125017_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125017_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125031_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125031_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125035_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125035_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125039_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125039_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125047_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125047_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 125070_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125070_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125072_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125072_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125078_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125078_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125080_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125080_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125084_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125084_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125086_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125086_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125087_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125087_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125094_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125094_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125097_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125097_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125109_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125109_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:36:33.79 +44:21:30.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.83, MAG_FAINT_SEARCH_LIMIT=14.81)GAIADR2_OUTPUT=# 0.996 964291115108615040 099.14062226965 +44.35833468971 13.7416 13.2256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.996#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125112_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125112_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125135_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125135_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125136_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125136_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:54:50.94 +45:12:07.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.72, MAG_FAINT_SEARCH_LIMIT=14.70)GAIADR2_OUTPUT=# 1.258 926296219499823616 118.71270074828 +45.20190976604 14.4283 13.8465 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.258#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125140_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125140_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:26:51.06 +44:27:34.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125158_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125158_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125177_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125177_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125180_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125180_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125181_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125181_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:42:08.17 +48:40:33.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125183_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125183_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125184_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125184_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:15:51.07 +41:03:08.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125192_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125192_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125193_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125193_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125201_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125201_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125203_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125203_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:54:46.32 +41:34:49.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125209_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125209_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125210_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125210_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125224_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125224_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125226_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125226_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125227_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125227_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125242_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125242_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 125248_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125248_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:33:01.15 +48:12:13.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.04, MAG_FAINT_SEARCH_LIMIT=15.02)GAIADR2_OUTPUT=# 3.826 967380948940582016 098.25319824916 +48.20379065206 13.7278 12.9383 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.826#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125250_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125250_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 125252_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125252_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 125254_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125254_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 125258_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125258_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
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Considering the candidate 125261_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125261_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 125263_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125263_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 125264_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125264_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 125274_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125274_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 125280_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125280_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 125281_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125281_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 125282_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125282_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 125283_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125283_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 125285_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125285_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 125290_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125290_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 125295_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125295_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 125299_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125299_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 125305_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125305_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.9") between the two second-epoch detections
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Considering the candidate 125308_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125308_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:12:29.31 +43:54:56.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.16, MAG_FAINT_SEARCH_LIMIT=15.14)GAIADR2_OUTPUT=# 1.491 950099787247631744 108.12269529903 +43.91569819087 14.3313 13.7929 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.491#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125309_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125309_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 125315_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125315_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 125320_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125320_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 125323_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125323_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:43:31.04 +41:46:54.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 2.239 957762421220809472 100.87913832177 +41.78114529924 14.0818 13.3524 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125337_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125337_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
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Considering the candidate 125340_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125340_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 125365_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125365_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
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Considering the candidate 125366_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125366_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 125369_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125369_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:01:41.06 +48:21:09.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 0.450 978615380796673280 105.42127061197 +48.35271114431 14.4235 13.8079 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.450#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 125384_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125384_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 125403_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125403_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:10:54.43 +49:54:11.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125409_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125409_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
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Considering the candidate 125420_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125420_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
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Considering the candidate 125425_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125425_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 125430_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125430_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125431_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125431_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:19:55.30 +41:05:05.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.38, MAG_FAINT_SEARCH_LIMIT=15.36)GAIADR2_OUTPUT=# 2.877 948492674909269376 109.98079415707 +41.08408654698 14.5411 14.0026 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.877#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125438_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125438_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 125442_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125442_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 125445_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125445_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125448_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125448_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125461_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125461_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125462_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125462_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125465_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125465_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125466_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125466_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125467_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125467_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125479_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125479_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125481_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125481_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:42:57.20 +41:51:20.4 in Gaia DR2 blend (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)
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Considering the candidate 125484_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125484_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125491_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125491_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 125500_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125500_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125502_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125502_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125503_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125503_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125509_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125509_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125519_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125519_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125543_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125543_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 125550_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125550_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:12:29.06 +45:14:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125551_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125551_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.8") between the two second-epoch detections
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Considering the candidate 125567_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125567_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:51:33.30 +44:03:45.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 1.039 925956229888964224 117.88837547363 +44.06245141488 14.6188 14.0581 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.039#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125575_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125575_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:09:48.65 +46:26:06.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 125604_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125604_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:37:42.38 +45:07:57.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 3.605 964702435536710016 099.42609181856 +45.13175485891 14.6657 14.1544 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.605#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 125613_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125613_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 125617_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125617_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.1") between the two second-epoch detections
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Considering the candidate 125619_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125619_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 125627_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125627_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 125651_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125651_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 125687_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 125687_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.6") between the two second-epoch detections
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Considering the candidate 116159_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 116159_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:41:06.82 +50:15:35.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 116292_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 116292_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:51:42.44 +49:23:04.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 102375_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 102375_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 06:41:13.13 +44:10:00.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21640_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 21640_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.3") between the two second-epoch detections
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Considering the candidate 62265_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 62265_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
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Considering the candidate 117160_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 117160_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (24.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 24471_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 24471_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:56:51.14 +47:45:18.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 28714_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 28714_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
Rejecting candidate due to large distance (22.4") between the two second-epoch detections
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Considering the candidate 98184_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 98184_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:52:06.26 +42:53:58.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 1.653 925557863081657216 118.02658424000 +42.89922411427 13.8497 13.3572 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.653#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 52210_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
The candidate 52210_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121 did not pass the final checks
**** FOUND 07:21:09.55 +45:48:15.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 03686_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
Preparing report for the candidate 03686_fd_Lyn-03-Q2b1x1_2026-03-19_22-50-01_20.00sec_-15.00C_LIGHT_0121
make_report_in_HTML.sh Phase 2 (HTML assembly): 7s
make_report_in_HTML.sh TOTAL: 119s
Prepared the HTML report for the field Lyn-03-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:59:05.11 +49:55:14.6
06:29:19.49 +48:32:59.2
06:30:18.71 +50:34:03.2
06:26:40.43 +47:21:13.4
06:26:35.13 +48:21:30.0
06:26:30.12 +49:56:22.6
06:36:17.88 +50:39:04.1
06:26:29.17 +49:04:09.3
06:30:32.00 +49:04:53.6
06:31:20.71 +50:09:43.5
06:28:52.06 +50:31:19.1
06:26:50.66 +49:02:21.1
06:30:32.38 +49:37:46.5
06:27:32.07 +48:51:10.0
06:25:09.87 +49:20:02.8
06:26:23.24 +49:11:35.7
06:31:22.74 +50:08:11.7
06:27:16.11 +48:54:33.0
06:26:01.26 +49:32:47.3
06:29:31.20 +50:34:58.9
06:30:54.22 +50:40:59.0
06:26:49.18 +48:51:59.4
06:25:08.96 +49:08:26.6
06:28:02.54 +50:32:59.6
06:31:01.21 +50:28:48.7
06:28:20.85 +49:53:35.5
06:26:56.05 +48:21:08.6
06:27:10.52 +47:02:32.2
06:26:35.07 +50:34:33.6
06:30:22.92 +49:10:00.1
06:31:07.47 +50:39:24.7
06:26:30.67 +50:02:42.8
06:28:08.99 +49:21:05.5
06:25:52.65 +49:39:06.5
06:25:09.53 +49:52:38.3
06:29:04.45 +49:48:46.3
06:27:26.70 +50:32:51.2
06:31:08.43 +50:06:11.0
06:27:38.01 +48:53:33.2
06:26:22.04 +47:49:03.4
06:26:36.61 +48:19:43.3
06:26:11.82 +50:26:18.0
06:26:03.74 +48:05:03.9
########### Completed Lyn-03-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
06:29:19.49 +48:32:59.2
06:30:18.71 +50:34:03.2
06:26:40.43 +47:21:13.4
06:26:35.13 +48:21:30.0
06:26:30.12 +49:56:22.6
06:36:17.88 +50:39:04.1
06:26:29.17 +49:04:09.3
06:30:32.00 +49:04:53.6
06:31:20.71 +50:09:43.5
06:28:52.06 +50:31:19.1
06:26:50.66 +49:02:21.1
06:30:32.38 +49:37:46.5
06:27:32.07 +48:51:10.0
06:25:09.87 +49:20:02.8
06:26:23.24 +49:11:35.7
06:31:22.74 +50:08:11.7
06:27:16.11 +48:54:33.0
06:26:01.26 +49:32:47.3
06:29:31.20 +50:34:58.9
06:30:54.22 +50:40:59.0
06:26:49.18 +48:51:59.4
06:25:08.96 +49:08:26.6
06:28:02.54 +50:32:59.6
06:31:01.21 +50:28:48.7
06:28:20.85 +49:53:35.5
06:26:56.05 +48:21:08.6
06:27:10.52 +47:02:32.2
06:26:35.07 +50:34:33.6
06:30:22.92 +49:10:00.1
06:31:07.47 +50:39:24.7
06:26:30.67 +50:02:42.8
06:28:08.99 +49:21:05.5
06:25:52.65 +49:39:06.5
06:25:09.53 +49:52:38.3
06:29:04.45 +49:48:46.3
06:27:26.70 +50:32:51.2
06:31:08.43 +50:06:11.0
06:27:38.01 +48:53:33.2
06:26:22.04 +47:49:03.4
06:26:36.61 +48:19:43.3
06:26:11.82 +50:26:18.0
06:26:03.74 +48:05:03.9
07:59:05.11 +49:55:14.6
###################################################################################
06:29:19.49 +48:32:59.2 -- not an asteroid (will add it to exclusion list)
06:30:18.71 +50:34:03.2 -- not an asteroid (will add it to exclusion list)
06:26:40.43 +47:21:13.4 -- not an asteroid (will add it to exclusion list)
06:26:35.13 +48:21:30.0 -- not an asteroid (will add it to exclusion list)
06:26:30.12 +49:56:22.6 -- not an asteroid (will add it to exclusion list)
06:36:17.88 +50:39:04.1 -- not an asteroid (will add it to exclusion list)
06:26:29.17 +49:04:09.3 -- not an asteroid (will add it to exclusion list)
06:30:32.00 +49:04:53.6 -- not an asteroid (will add it to exclusion list)
06:31:20.71 +50:09:43.5 -- not an asteroid (will add it to exclusion list)
06:28:52.06 +50:31:19.1 -- not an asteroid (will add it to exclusion list)
06:26:50.66 +49:02:21.1 -- not an asteroid (will add it to exclusion list)
06:30:32.38 +49:37:46.5 -- not an asteroid (will add it to exclusion list)
06:27:32.07 +48:51:10.0 -- not an asteroid (will add it to exclusion list)
06:25:09.87 +49:20:02.8 -- not an asteroid (will add it to exclusion list)
06:26:23.24 +49:11:35.7 -- not an asteroid (will add it to exclusion list)
06:31:22.74 +50:08:11.7 -- not an asteroid (will add it to exclusion list)
06:27:16.11 +48:54:33.0 -- not an asteroid (will add it to exclusion list)
06:26:01.26 +49:32:47.3 -- not an asteroid (will add it to exclusion list)
06:29:31.20 +50:34:58.9 -- not an asteroid (will add it to exclusion list)
06:30:54.22 +50:40:59.0 -- not an asteroid (will add it to exclusion list)
06:26:49.18 +48:51:59.4 -- not an asteroid (will add it to exclusion list)
06:25:08.96 +49:08:26.6 -- not an asteroid (will add it to exclusion list)
06:28:02.54 +50:32:59.6 -- not an asteroid (will add it to exclusion list)
06:31:01.21 +50:28:48.7 -- not an asteroid (will add it to exclusion list)
06:28:20.85 +49:53:35.5 -- not an asteroid (will add it to exclusion list)
06:26:56.05 +48:21:08.6 -- not an asteroid (will add it to exclusion list)
06:27:10.52 +47:02:32.2 -- not an asteroid (will add it to exclusion list)
06:26:35.07 +50:34:33.6 -- not an asteroid (will add it to exclusion list)
06:30:22.92 +49:10:00.1 -- not an asteroid (will add it to exclusion list)
06:31:07.47 +50:39:24.7 -- not an asteroid (will add it to exclusion list)
06:26:30.67 +50:02:42.8 -- not an asteroid (will add it to exclusion list)
06:28:08.99 +49:21:05.5 -- not an asteroid (will add it to exclusion list)
06:25:52.65 +49:39:06.5 -- not an asteroid (will add it to exclusion list)
06:25:09.53 +49:52:38.3 -- not an asteroid (will add it to exclusion list)
06:29:04.45 +49:48:46.3 -- not an asteroid (will add it to exclusion list)
06:27:26.70 +50:32:51.2 -- not an asteroid (will add it to exclusion list)
06:31:08.43 +50:06:11.0 -- not an asteroid (will add it to exclusion list)
06:27:38.01 +48:53:33.2 -- not an asteroid (will add it to exclusion list)
06:26:22.04 +47:49:03.4 -- not an asteroid (will add it to exclusion list)
06:26:36.61 +48:19:43.3 -- not an asteroid (will add it to exclusion list)
06:26:11.82 +50:26:18.0 -- not an asteroid (will add it to exclusion list)
06:26:03.74 +48:05:03.9 -- not an asteroid (will add it to exclusion list)
07:59:05.11 +49:55:14.6 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:25:08.96 +49:08:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:09.53 +49:52:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:09.87 +49:20:02.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:52.65 +49:39:06.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:01.26 +49:32:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:03.74 +48:05:03.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:11.82 +50:26:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:22.04 +47:49:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:23.24 +49:11:35.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:29.17 +49:04:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:30.12 +49:56:22.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:30.67 +50:02:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:35.07 +50:34:33.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:35.13 +48:21:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:36.61 +48:19:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:40.43 +47:21:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:49.18 +48:51:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:50.66 +49:02:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:26:56.05 +48:21:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:10.52 +47:02:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:16.11 +48:54:33.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:26.70 +50:32:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:32.07 +48:51:10.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:27:38.01 +48:53:33.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:02.54 +50:32:59.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:08.99 +49:21:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:20.85 +49:53:35.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:52.06 +50:31:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:04.45 +49:48:46.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:19.49 +48:32:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:29:31.20 +50:34:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:18.71 +50:34:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:22.92 +49:10:00.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:32.00 +49:04:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:32.38 +49:37:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:30:54.22 +50:40:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:01.21 +50:28:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:07.47 +50:39:24.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:08.43 +50:06:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:20.71 +50:09:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:22.74 +50:08:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:36:17.88 +50:39:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
07:59:05.11 +49:55:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
06:25:08.96 +49:08:26.6 -- not a known variable star
06:25:09.53 +49:52:38.3 -- not a known variable star
06:25:09.87 +49:20:02.8 -- not a known variable star
06:25:52.65 +49:39:06.5 -- not a known variable star
06:26:01.26 +49:32:47.3 -- not a known variable star
06:26:03.74 +48:05:03.9 -- not a known variable star
06:26:11.82 +50:26:18.0 -- not a known variable star
06:26:22.04 +47:49:03.4 -- not a known variable star
06:26:23.24 +49:11:35.7 -- not a known variable star
06:26:29.17 +49:04:09.3 -- not a known variable star
06:26:30.12 +49:56:22.6 -- not a known variable star
06:26:30.67 +50:02:42.8 -- not a known variable star
06:26:35.07 +50:34:33.6 -- not a known variable star
06:26:35.13 +48:21:30.0 -- not a known variable star
06:26:36.61 +48:19:43.3 -- not a known variable star
06:26:40.43 +47:21:13.4 -- not a known variable star
06:26:49.18 +48:51:59.4 -- not a known variable star
06:26:50.66 +49:02:21.1 -- not a known variable star
06:26:56.05 +48:21:08.6 -- not a known variable star
06:27:10.52 +47:02:32.2 -- not a known variable star
06:27:16.11 +48:54:33.0 -- not a known variable star
06:27:26.70 +50:32:51.2 -- not a known variable star
06:27:32.07 +48:51:10.0 -- not a known variable star
06:27:38.01 +48:53:33.2 -- not a known variable star
06:28:02.54 +50:32:59.6 -- not a known variable star
06:28:08.99 +49:21:05.5 -- not a known variable star
06:28:20.85 +49:53:35.5 -- not a known variable star
06:28:52.06 +50:31:19.1 -- not a known variable star
06:29:04.45 +49:48:46.3 -- not a known variable star
06:29:19.49 +48:32:59.2 -- not a known variable star
06:29:31.20 +50:34:58.9 -- not a known variable star
06:30:18.71 +50:34:03.2 -- not a known variable star
06:30:22.92 +49:10:00.1 -- not a known variable star
06:30:32.00 +49:04:53.6 -- not a known variable star
06:30:32.38 +49:37:46.5 -- not a known variable star
06:30:54.22 +50:40:59.0 -- not a known variable star
06:31:01.21 +50:28:48.7 -- not a known variable star
06:31:07.47 +50:39:24.7 -- not a known variable star
06:31:08.43 +50:06:11.0 -- not a known variable star
06:31:20.71 +50:09:43.5 -- not a known variable star
06:31:22.74 +50:08:11.7 -- not a known variable star
06:36:17.88 +50:39:04.1 -- not a known variable star
07:59:05.11 +49:55:14.6 -- not a known variable star
Found 43 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
43 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 43 (excluding asteroids and hot pixels), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is 500
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461119.65932591 -observatory 500
22:37:27.36 -07:27:00.9 Mercury (1.1mag)
01:02:45.08 +05:43:31.5 Venus (-3.9mag)
23:00:42.68 -07:29:41.2 Mars (1.2mag)
07:04:39.12 +22:58:08.5 Jupiter (-2.3mag)
00:16:57.85 -00:28:39.8 Saturn (0.9mag)
03:42:48.57 +19:31:27.0 Uranus (5.8mag)
00:07:10.37 -00:38:47.5 Neptune (7.8mag)
20:31:55.79 -22:53:54.7 Pluto (14.5mag)
00:45:26.34 +08:09:20.9 Moon (-8.4mag)
-rw-r--r-- 1 apache apache 361 Mar 19 23:05 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461119.65932591:
07:04:30.42 +22:58:25.2 Io (5.6mag)
07:04:40.43 +22:58:02.3 Europa (5.7mag)
07:04:28.57 +22:58:20.8 Ganymede (5.2mag)
07:04:09.99 +22:58:54.4 Callisto (6.4mag)
07:08:40.55 +23:00:14.9 Himalia (15.2mag)
07:04:35.52 +22:58:13.0 Thebe (16.0mag)
07:08:14.39 +23:23:09.1 Elara (17.1mag)
07:01:43.86 +23:52:16.3 Pasiphae (17.2mag)
07:13:27.22 +22:52:26.6 Carme (18.3mag)
00:16:49.76 -00:28:29.2 Titan (8.8mag)
00:16:57.42 -00:28:34.9 Rhea (10.1mag)
00:17:28.23 -00:26:41.1 Iapetus (11.5mag)
00:17:12.03 -00:28:48.1 Hyperion (14.8mag)
00:18:52.43 -00:17:19.6 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 19 23:05 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461119.65932591:
12:42:49.49 +09:44:30.7 JWST
19:33:09.87 +08:22:33.3 Chandra
16:11:54.29 -54:11:13.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 19 23:05 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461119.65932591 -observatory 500
18:34:41.64 -27:25:29.3 14.1mag P/2010 H2 (Vales)
04:50:46.62 -71:04:53.2 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:28:41.08 +31:17:41.8 17.0mag C/2017 K2 (PANSTARRS)
17:29:29.65 +07:18:14.5 17.6mag C/2021 G2 (ATLAS)
23:01:13.75 +28:25:12.4 16.9mag C/2022 E2 (ATLAS)
03:59:37.73 +25:16:12.0 15.7mag C/2022 N2 (PANSTARRS)
09:01:58.38 +31:24:54.3 16.0mag C/2022 QE78 (ATLAS)
08:30:16.20 -03:16:55.5 17.2mag C/2022 R6 (PANSTARRS)
18:56:28.37 +16:13:11.1 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:46:26.27 -11:51:11.3 17.6mag P/2023 B1 (PANSTARRS)
09:25:14.26 -16:28:34.0 17.4mag C/2023 F3 (ATLAS)
21:20:26.06 +61:40:09.6 17.4mag C/2023 H5 (Lemmon)
19:33:24.54 -03:31:04.5 14.5mag C/2023 R1 (PANSTARRS)
21:35:38.00 +82:46:46.3 17.7mag C/2023 X2 (Lemmon)
06:15:41.37 +63:47:50.1 16.8mag C/2024 A1 (ATLAS)
04:03:41.08 +04:34:14.9 9.0mag C/2024 E1 (Wierzchos)
11:23:20.10 +02:33:50.9 18.0mag C/2024 G2 (ATLAS)
16:32:33.77 +02:01:58.9 17.5mag C/2024 G6 (ATLAS)
20:09:36.53 +08:34:22.8 14.9mag C/2024 J3 (ATLAS)
03:04:04.12 -26:48:04.1 16.5mag C/2024 T5 (ATLAS)
04:57:03.14 +52:52:29.2 17.6mag C/2025 J1 (Borisov)
15:16:01.05 +16:19:50.5 14.4mag C/2025 L1 (ATLAS)
02:47:28.99 -22:28:16.0 17.6mag C/2025 Q3 (ATLAS)
22:32:22.51 +18:57:27.4 12.6mag C/2025 R3 (PANSTARRS)
13:05:23.08 +01:15:22.6 17.7mag C/2025 Y1 (ATLAS)
02:11:50.61 -06:51:56.2 14.3mag C/2026 A1 (MAPS)
22:36:04.76 +30:47:19.6 13.7mag C/2026 B2 (Sun-Gao)
17:50:25.59 -10:51:54.1 13.4mag 10P/Tempel
15:27:10.48 +05:10:46.8 11.7mag 24P/Schaumasse
11:12:21.08 -02:30:48.5 15.6mag 29P/Schwassmann-Wachmann
17:42:47.46 -10:40:38.6 17.3mag 40P/Vaisala
10:45:35.74 -06:39:09.6 16.4mag 43P/Wolf-Harrington
01:07:41.72 +12:46:18.2 17.0mag 47P/Ashbrook-Jackson
06:27:28.08 +42:30:55.5 17.1mag 63P/Wild
22:53:01.03 -14:51:11.8 15.7mag 65P/Gunn
02:56:31.35 +10:58:18.1 15.9mag 76P/West-Kohoutek-Ikemura
00:07:44.94 +02:52:52.3 14.7mag 78P/Gehrels
21:35:50.31 -16:57:34.2 14.5mag 88P/Howell
00:58:38.44 +12:58:33.6 15.3mag 93P/Lovas
04:09:20.82 +30:37:43.9 16.5mag 123P/West-Hartley
08:07:34.18 +50:38:20.5 16.2mag 124P/Mrkos
01:53:07.76 +11:15:14.6 16.4mag 128P/Shoemaker-Holt
01:55:48.70 +10:54:46.6 17.4mag 131P/Mueller
23:16:25.17 +02:45:46.4 13.1mag 141P/Machholz
23:26:29.35 -04:41:56.8 13.1mag 141P-A/Machholz
22:27:47.17 -07:11:03.0 16.2mag 141P-D/Machholz
23:48:04.57 -14:32:01.8 15.5mag 162P/SidingSpring
10:39:56.58 +32:02:13.8 17.5mag 164P/Christensen
05:48:17.52 +24:44:27.2 17.5mag 198P/ODAS
15:34:24.52 -03:29:21.5 16.9mag 210P/Christensen
20:08:36.00 -17:43:29.5 17.1mag 218P/LINEAR
16:58:22.27 -16:44:51.0 16.3mag 235P/LINEAR
04:39:51.22 +31:53:16.3 16.3mag 240P/NEAT
07:29:45.43 -08:29:17.6 17.5mag 242P/Spahr
15:48:36.78 +05:02:29.9 17.7mag 391P/Kowalski
07:27:55.70 +21:05:34.5 17.5mag 450P/LONEOS
04:59:57.08 +46:40:20.1 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 19 23:05 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
11:44:44.19 -62:10:45.50 ASASSN-26bq 2026-03-15.03 15.31
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 -0.22
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.41 -74:35:46.80 AT2026ahr 2026-01-20.09 16.98
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:25.13 +04:00:01.40 SN 2026kc 2026-01-18.24 16.4
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
-rw-r--r-- 1 apache apache 5.7K Mar 19 23:05 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 19 23:05 tocp_transients_list.txt