This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62
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 20.1606 2461119.6606 14.21 07:04:36.70 +41:40:51.8
175.42589 19.96269 galactic Aur Second-epoch detections are separated by 2.9" 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 | target | 07:04:36.70 +41:40:51.8 (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,2461119.6606,14.21,0.05,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 20260320.1606 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-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:04:36.70 +41:40:51.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1606 2461119.6606 14.12 06:58:11.32 +40:07:46.1
176.53752 18.29625 galactic Aur Second-epoch detections are separated by 4.5" and 5.3 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 | 06:58:11.32 +40:07:46.1 (user input) | T | P | (position from user input) 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
target,2461119.6606,14.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1606 14.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:58:11.32 +40:07:46.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 950924455328252800,2461119.6606,14.16,0.05,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
Gaia DR3 950924455328252800 20260320.1606 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-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:00:13.58 +41:12:19.6 ;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-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_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,2461119.6606,14.02,0.05,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 20260320.1606 14.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:01:47.41 +42:48:16.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1606 2461119.6606 13.96 07:00:13.65 +41:34:38.5
175.24137 19.15542 galactic Aur Second-epoch detections are separated by 3.8" 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 J105.0587+41.5783 | 07:00:13.65 +41:34:38.5 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: G5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.0587+41.5783,2461119.6606,13.96,0.05,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
ATO J105.0587+41.5783 20260320.1606 13.96CV 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-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:00:13.65 +41:34:38.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_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,2461119.6606,13.85,0.05,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
target 20260320.1606 13.85CV 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-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:59:08.44 +42:16:19.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1606 2461119.6606 13.93 06:59:57.13 +41:44:16.9
175.06288 19.16115 galactic Aur Second-epoch detections are separated by 1.5" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.9835+41.7383 | 06:59:57.13 +41:44:16.9 (user input) | dubious (ATLAS) | (ATLAS) | (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
ATO J104.9835+41.7383,2461119.6606,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.9835+41.7383 20260320.1606 13.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:59:57.13 +41:44:16.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1606 2461119.6606 14.04 06:59:24.84 +42:36:47.3
174.15411 19.36055 galactic Aur Second-epoch detections are separated by 3.8" 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 | 06:59:24.84 +42:36:47.3 (user input) | T | P | (position from user input) SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6606,14.04,0.05,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
target 20260320.1606 14.04CV 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-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:59:24.84 +42:36:47.3 ;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-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1606 2461119.6606 13.84 06:59:14.44 +42:28:19.1
174.28381 19.28330 galactic Aur Second-epoch detections are separated by 2.8" 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 | ATO J104.8066+42.4722 | 06:59:14.44 +42:28:19.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.8066+42.4722,2461119.6606,13.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.8066+42.4722 20260320.1606 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:59:14.44 +42:28:19.1 ;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-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1606 2461119.6606 13.65 06:59:34.31 +42:23:12.6
174.39047 19.31241 galactic Aur Second-epoch detections are separated by 2.1" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J104.8886+42.3868 | 06:59:34.31 +42:23:12.6 (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 J104.8886+42.3868,2461119.6606,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J104.8886+42.3868 20260320.1606 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:59:34.31 +42:23:12.6 ;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-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1606 2461119.6606 13.82 06:58:37.72 +40:53:59.4
175.80636 18.64195 galactic Aur Second-epoch detections are separated by 1.3" 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 | ATO J104.6546+40.8996 | 06:58:37.72 +40:53:59.4 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) SpType: C-H 2016ApJS..226....1J LAMOST J065837.12+405358.8
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.6546+40.8996,2461119.6606,13.82,0.05,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
ATO J104.6546+40.8996 20260320.1606 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:58:37.72 +40:53:59.4 ;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-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_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,2461119.6606,13.65,0.05,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 20260320.1606 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:57:33.47 +42:20:05.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_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,2461119.6606,13.76,0.05,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 20260320.1606 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:58:50.06 +41:17:45.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 951182664465923584,2461119.6606,13.70,0.05,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 951182664465923584 20260320.1606 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:57:37.51 +41:45:12.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1606 2461119.6606 13.25 07:01:02.91 +42:29:41.3
174.37846 19.60524 galactic Aur Second-epoch detections are separated by 7.4" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J105.2599+42.4951 | 07:01:02.91 +42:29:41.3 (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 J105.2599+42.4951,2461119.6606,13.25,0.05,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 J105.2599+42.4951 20260320.1606 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:01:02.91 +42:29:41.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1606 2461119.6606 13.37 06:57:57.84 +41:00:03.5
175.66052 18.55904 galactic Aur Second-epoch detections are separated by 4.2" 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 | ATO J104.4939+41.0009 | 06:57:58.55 +41:00:03.4 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | 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
ATO J104.4939+41.0009,2461119.6606,13.37,0.05,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
ATO J104.4939+41.0009 20260320.1606 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-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:57:57.84 +41:00:03.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1606 2461119.6606 13.11 06:58:21.61 +41:26:07.1
175.25707 18.77836 galactic Aur Second-epoch detections are separated by 3.5" 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 J104.5776+41.4361 | 06:58:20.54 +41:26:08.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J104.5776+41.4361,2461119.6606,13.11,0.05,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
ATO J104.5776+41.4361 20260320.1606 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-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:58:21.61 +41:26:07.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1606 2461119.6606 12.58 07:01:08.31 +42:16:54.5
174.59765 19.55050 galactic Aur Second-epoch detections are separated by 2.8" 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 951259973877805824 | 07:01:08.91 +42:16:54.2 (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 951259973877805824,2461119.6606,12.58,0.05,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 951259973877805824 20260320.1606 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:01:08.31 +42:16:54.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1606 2461119.6606 12.74 07:00:34.89 +42:41:04.2
174.15827 19.58674 galactic Aur Second-epoch detections are separated by 1.0" 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 | Gaia DR3 951304504098723968 | 07:00:34.06 +42:41:05.3 (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 951304504098723968,2461119.6606,12.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 951304504098723968 20260320.1606 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:00:34.89 +42:41:04.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1606 2461119.6606 12.66 07:00:00.28 +42:27:21.9
174.34952 19.41081 galactic Aur Second-epoch detections are separated by 1.1" 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 | ATO J105.0038+42.4560 | 07:00:00.92 +42:27:21.6 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE SpType: G7 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J105.0038+42.4560,2461119.6606,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J105.0038+42.4560 20260320.1606 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:00:00.28 +42:27:21.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1606 2461119.6606 12.62 06:57:50.26 +42:33:23.0
174.10762 19.06817 galactic Aur Second-epoch detections are separated by 0.2" 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 | Gaia DR3 951334637589037440 | 06:57:49.31 +42:33:25.4 (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 951334637589037440,2461119.6606,12.62,0.05,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
Gaia DR3 951334637589037440 20260320.1606 12.62CV 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-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:57:50.26 +42:33:23.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1606 2461119.6606 12.72 07:02:00.21 +42:51:49.2
174.06939 19.89202 galactic Aur Second-epoch detections are separated by 3.0" 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 | ATO J105.5164+42.8591 | 07:02:01.00 +42:51:48.6 (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 J105.5164+42.8591,2461119.6606,12.72,0.05,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
ATO J105.5164+42.8591 20260320.1606 12.72CV 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-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:02:00.21 +42:51:49.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1606 2461119.6606 12.42 07:04:56.75 +42:43:47.4
174.38972 20.35976 galactic Aur Second-epoch detections are separated by 0.6" 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 J106.2339+42.7299 | 07:04:56.13 +42:43:47.8 (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 J106.2339+42.7299,2461119.6606,12.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J106.2339+42.7299 20260320.1606 12.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:04:56.75 +42:43:47.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1606 2461119.6606 12.35 06:57:03.90 +42:41:58.5
173.91424 18.98284 galactic Aur Second-epoch detections are separated by 3.0" 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 | Gaia DR3 952089967717253504 | 06:57:02.85 +42:42:01.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G7 (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 952089967717253504,2461119.6606,12.35,0.05,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
Gaia DR3 952089967717253504 20260320.1606 12.35CV 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-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:57:03.90 +42:41:58.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6606,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260320.1606 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:26:37.51 +36:50:59.2 ;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-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_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,2461119.6606,14.28,0.05,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 20260320.1606 14.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:59:08.87 +33:11:12.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461119.6606,14.21,0.05,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
VARIABLE_NAME 20260320.1606 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-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:44:51.90 +34:34:38.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20_00sec_-15_00C_LIGHT_0123_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20_00sec_-15_00C_LIGHT_0498_fits__*pix.png resample_wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20_00sec_-15_00C_LIGHT_0122_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.89788103 23.12.2025 09:32:46.921 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
First image: 2461032.89788103 23.12.2025 09:32:46.921 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Last image: 2461119.66091287 20.03.2026 03:51:32.872 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 15
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.49
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 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): 17963
Objects passed selection criteria: 17956
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: 17292
Average stars matched: 16756.5 (96.9032 %)
Memory usage VmPeak: 121900 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 23:11:40 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.89788103 23.12.2025 09:32:46.921 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
First image: 2461032.89788103 23.12.2025 09:32:46.921 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Last image: 2461119.66091287 20.03.2026 03:51:32.872 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 347
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.24
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 39 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): 99295
Objects passed selection criteria: 99046
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: 94843
Average stars matched: 91489.8 (96.4644 %)
Memory usage VmPeak: 1925648 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 23:13:09 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-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
SExtractor catalog cache: saved Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat to cache
SExtractor catalog cache: saved Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.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: 2461119.66037281
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits exists and is non-empty
Saving wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits to local_wcs_cache/
'wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits' -> 'local_wcs_cache/wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits'
wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits exists and is non-empty
Saving wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits to local_wcs_cache/
'wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits' -> 'local_wcs_cache/wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits'
wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits exists and is non-empty
Saving wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits to local_wcs_cache/
'wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits' -> 'local_wcs_cache/wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits'
wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits exists and is non-empty
Saving wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits to local_wcs_cache/
'wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits' -> 'local_wcs_cache/wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits'
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:38:10.768 +37:59:37.83
Second-epoch image center 07:38:11.931 +38:02:50.61
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:38:10.768 +37:59:37.83
Second-epoch image center 07:38:13.730 +38:02:36.88
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 07:38:11.931 +38:02:50.61
Second-epoch second image center 07:38:13.730 +38:02:36.88
Angular distance between the image centers 0.00703 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits &> /tmp/tmp.Mo3IzcqrTG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits &> /tmp/tmp.hBgWGZuydP
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits &> /tmp/tmp.YvdyylqFUk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits &> /tmp/tmp.TcWP3RMhNC
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
Found non-empty wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
The reference image (wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits) and catalog (wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat) found
'wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 7689 out of 17251 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.958948
a=0.000000 b=1.000000 c=22.958948
From vast_summary.log: estimated ref. image limiting mag.: -7.49
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.47
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.47
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 11 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.2 pix Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
2.2 pix Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
2.5 pix fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
2.5 pix fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
Limiting magnitude estimates:
15.5 mag. Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
15.5 mag. Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
15.4 mag. fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
15.4 mag. fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
All-image limiting magnitude estimate: 15.4 (SNR ) 12.4 (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.Mo3IzcqrTG (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits' -> 'wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS-calibrated image found: wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Checking if the catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS catalog name: wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1370, passed=17251
Got 17251 stars (including 15857 good ones) from the SExtractor catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
util/solve_plate_with_UCAC5 got 17251 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.33"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 957 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.31"
Excluding outliers - 957 stars left (next iteration limit 1052)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits -region wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.hBgWGZuydP (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits' -> 'wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS-calibrated image found: wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Checking if the catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS catalog name: wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1310, passed=17199
Got 17199 stars (including 15864 good ones) from the SExtractor catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat
util/solve_plate_with_UCAC5 got 17199 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.32"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.32"
Estimated accuracy of the plate solution: 0.32"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits -region wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.YvdyylqFUk (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
Checking if the catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
WCS catalog name: wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1200, passed=17563
Got 17563 stars (including 16349 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits.cat
util/solve_plate_with_UCAC5 got 17563 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 960 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: 0.61"
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 960 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.61"
Estimated accuracy of the plate solution: 0.67"
Excluding outliers - 960 stars left (next iteration limit 1056)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits -region wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.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.TcWP3RMhNC (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
Checking if the catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
WCS catalog name: wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1203, passed=17581
Got 17581 stars (including 16364 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits.cat
util/solve_plate_with_UCAC5 got 17581 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 959 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: 0.62"
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 959 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: 0.67"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits -region wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits'
Saving fully-calibrated image wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits'
Saving fully-calibrated image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits'
Saving fully-calibrated image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits'
Preparing the HTML report for the field Lyn-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21028.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21035.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21036.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21038.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21042.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21048.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 4s
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 20992_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 20992_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 08:01:58.03 +34:06:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 21023_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 21023_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:37:58.99 +38:15:21.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.580 899191952204777088 114.49560672269 +38.25598548639 12.0838 11.3902 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.580#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21028_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 21028_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 08:15:59.30 +40:33:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.17, MAG_FAINT_SEARCH_LIMIT=13.15)GAIADR2_OUTPUT=# 1.110 909597451076271616 123.99718016312 +40.55025617771 12.1973 11.5278 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21035_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 21035_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:44:34.49 +36:39:10.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.38, MAG_FAINT_SEARCH_LIMIT=13.36)GAIADR2_OUTPUT=# 0.733 895798133471620480 116.14352907060 +36.65311620114 12.2565 11.7290 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21036_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 21036_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:48:01.95 +35:33:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 1.403 894744874347796736 117.00784914445 +35.56006874295 12.3160 11.8922 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.403#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21038_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 21038_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:30:59.14 +40:46:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 0.954 900619148361502464 112.74666567674 +40.78292485671 12.4463 12.0056 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21042_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 21042_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:30:03.30 +40:06:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 0.348 900295960663112576 112.51385072492 +40.11108033709 12.4565 12.0460 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.348#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21043_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 21043_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:40:48.15 +38:01:06.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.47, MAG_FAINT_SEARCH_LIMIT=13.45)GAIADR2_OUTPUT=# 0.080 896162110476546432 115.20059798054 +38.01832727929 12.2808 11.7008 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.080#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21044_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 21044_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:42:27.90 +38:02:41.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 0.321 896138780214166144 115.61617024945 +38.04503556134 12.3756 11.9030 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.321#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21048_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 21048_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:46:58.23 +41:40:30.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.54, MAG_FAINT_SEARCH_LIMIT=13.52)GAIADR2_OUTPUT=# 1.777 923939656843716992 116.74247141751 +41.67561902418 12.3767 11.7814 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.777#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 14539_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 14539_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:26:13.75 +33:22:24.8 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 5s
Prepared the HTML report for the field Lyn-05-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
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-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
SExtractor catalog cache: saved Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat to cache
SExtractor catalog cache: saved Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Creating symlink local_wcs_cache/wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.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-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits exists and is non-empty
wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits exists and is non-empty
wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits exists and is non-empty
wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits exists and is non-empty
The image scale is 5.90"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.9" and 8.9"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 07:38:10.768 +37:59:37.83
Second-epoch image center 07:38:11.931 +38:02:50.61
Angular distance between the image centers 0.05 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 07:38:10.768 +37:59:37.83
Second-epoch image center 07:38:13.730 +38:02:36.88
Angular distance between the image centers 0.05 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 07:38:11.931 +38:02:50.61
Second-epoch second image center 07:38:13.730 +38:02:36.88
Angular distance between the image centers 0.00703 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits &> /tmp/tmp.MxsATQvKF5
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits &> /tmp/tmp.m5jOrC7xTG
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits &> /tmp/tmp.KBefqmOyeB
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits &> /tmp/tmp.lzWJ51CB2K
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
Found non-empty wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits and wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
The reference image (wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits) and catalog (wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat) found
'wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 7746 out of 100375 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.850461
a=0.000000 b=1.000000 c=22.850461
From vast_summary.log: estimated ref. image limiting mag.: -7.24
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.61
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.61
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 122 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
2.0 pix Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
2.3 pix fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
2.4 pix fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
Limiting magnitude estimates:
15.6 mag. Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
15.6 mag. Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
15.5 mag. fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
15.5 mag. fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.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.MxsATQvKF5 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits' -> 'wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS-calibrated image found: wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Checking if the catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
WCS catalog name: wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=25, blended=7665, passed=100350
Got 100350 stars (including 92512 good ones) from the SExtractor catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat
util/solve_plate_with_UCAC5 got 100350 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 953 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.33"
Excluding outliers - 953 stars left (next iteration limit 1048)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits -region wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.m5jOrC7xTG (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits' -> 'wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS_IMAGE_NAME=wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS-calibrated image found: wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Checking if the catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits alredy exist and is non-empty...
Catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat corresponding to the image wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
WCS catalog name: wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=26, blended=7582, passed=100415
Got 100415 stars (including 92657 good ones) from the SExtractor catalog wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat
util/solve_plate_with_UCAC5 got 100415 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.3'
Seting catalog search parameters based on the expected field of view 941.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013074 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010459 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.34"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 951 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.34"
Estimated accuracy of the plate solution: 0.34"
Excluding outliers - 951 stars left (next iteration limit 1046)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits -region wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.KBefqmOyeB (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
Checking if the catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
WCS catalog name: wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=37, blended=7663, passed=90605
Got 90605 stars (including 82841 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits.cat
util/solve_plate_with_UCAC5 got 90605 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.62"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.59"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 956 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.59"
Estimated accuracy of the plate solution: 0.63"
Excluding outliers - 956 stars left (next iteration limit 1051)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits -region wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.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.lzWJ51CB2K (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
WCS-calibrated image found: wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
Checking if the catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits.cat corresponding to the image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
WCS catalog name: wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=43, blended=7555, passed=90673
Got 90673 stars (including 83028 good ones) from the SExtractor catalog wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits.cat
util/solve_plate_with_UCAC5 got 90673 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.0'
Seting catalog search parameters based on the expected field of view 937.0 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013014 (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 0.010411 (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 959 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: 0.61"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 959 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.57"
Estimated accuracy of the plate solution: 0.62"
Excluding outliers - 959 stars left (next iteration limit 1054)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits -region wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/wcs_Lyn-05-Q2b1x1_2025-12-23_03-32-46_20.00sec_-15.00C_LIGHT_0498.fits
Saving fully-calibrated image wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/wcs_Lyn-05-Q2b1x1_2025-12-23_03-33-36_20.00sec_-14.90C_LIGHT_0499.fits
Saving fully-calibrated image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-50-46_20.00sec_-15.00C_LIGHT_0122.fits
Saving fully-calibrated image wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Lyn-05-Q2b1x1_230542_TTUQ2b1x1_970_lLhzGE62/wcs_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123.fits
Preparing the HTML report for the field Lyn-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out118175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118185.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118191.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118204.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118211.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118215.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118219.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118225.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118231.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118234.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118248.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118256.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118266.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118270.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118272.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118282.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118286.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118291.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118292.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118295.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118304.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118311.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118349.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118352.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118355.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118357.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118366.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118368.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118405.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118408.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118409.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118411.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118415.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118426.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118439.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118455.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118456.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118458.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118460.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118461.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118462.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118529.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118770.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118782.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118891.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118920.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out118980.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119011.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119012.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119016.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out119071.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out118421.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out118252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118264.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118283.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118329.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118333.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118336.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118361.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118367.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118384.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118386.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118416.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118429.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118432.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118437.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118440.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118447.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out118959.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 48s
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: 15s
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Considering the candidate 118175_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118175_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:03:34.59 +41:55:12.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 5.487 951050482553580800 105.89617306309 +41.92022164027 13.9000 13.3919 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.487#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118185_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118185_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:02:41.84 +42:28:01.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 3.941 951101545419814784 105.67288333484 +42.46739915152 13.8487 13.2982 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.941#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118188_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118188_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:20:50.64 +39:07:25.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.48, MAG_FAINT_SEARCH_LIMIT=15.46)GAIADR2_OUTPUT=# 1.645 900005659528763904 110.21136640972 +39.12325323688 14.6051 13.9820 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118191_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118191_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:01:18.81 +33:25:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 0.989 891089066905724800 105.32856199873 +33.42174614866 13.9085 13.2801 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118204_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118204_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:00:40.98 +40:45:04.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.37, MAG_FAINT_SEARCH_LIMIT=15.35)GAIADR2_OUTPUT=# 2.463 950893840801391872 105.17133578043 +40.75163198416 13.8630 13.3213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.463#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118211_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118211_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:30:22.66 +42:21:20.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.28, MAG_FAINT_SEARCH_LIMIT=15.26)GAIADR2_OUTPUT=# 0.915 972814632326971520 112.59408884506 +42.35561715172 14.0905 13.5812 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.915#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118215_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118215_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:11:41.34 +42:43:52.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 3.224 949616723685836672 107.92344444529 +42.73137347506 13.6866 13.2239 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118219_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118219_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:03:09.38 +41:45:03.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.35, MAG_FAINT_SEARCH_LIMIT=15.33)GAIADR2_OUTPUT=# 4.591 951042171792009984 105.78737644907 +41.75081968565 13.6172 12.8568 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.591#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118225_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118225_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:07:11.40 +42:27:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.29, MAG_FAINT_SEARCH_LIMIT=15.27)GAIADR2_OUTPUT=# 3.164 952552797689662976 106.79630885714 +42.46523090230 13.6548 13.0506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.164#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118226_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118226_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 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 118231_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118231_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 06:59:48.53 +42:33:04.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.31, MAG_FAINT_SEARCH_LIMIT=15.29)GAIADR2_OUTPUT=# 3.764 951326258109758080 104.95362585033 +42.55135504862 13.6349 12.9898 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.764#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118234_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118234_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:01:38.68 +42:22:07.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.18, MAG_FAINT_SEARCH_LIMIT=15.16)GAIADR2_OUTPUT=# 2.896 951284682826398464 105.41033469433 +42.36825898790 13.5771 12.9667 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.896#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118235_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118235_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:18:55.73 +33:56:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.34, MAG_FAINT_SEARCH_LIMIT=15.32)GAIADR2_OUTPUT=# 1.983 896348924373702912 109.73285536944 +33.94104048449 14.4818 13.8850 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.983#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118248_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118248_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 06:58:35.24 +40:13:38.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 2.503 950482928395043200 104.64592382363 +40.22738179654 13.3170 12.6232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.503#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118252_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118252_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118255_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118255_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118256_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118256_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:00:23.87 +42:00:33.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 5.890 951168615629853568 105.10158101158 +42.00974040246 13.2180 12.4914 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.890#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118264_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118264_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118266_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118266_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:00:13.15 +39:24:51.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 5.575 947394434591990528 105.05678936906 +39.41445917582 13.5261 13.0213 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.575#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118267_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118267_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 06:59:50.67 +42:25:37.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118270_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118270_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:01:35.40 +41:19:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 4.645 950936098984318464 105.39902521384 +41.31912167775 13.2781 12.6194 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.645#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118272_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118272_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 06:57:53.96 +41:26:15.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.03, MAG_FAINT_SEARCH_LIMIT=15.01)GAIADR2_OUTPUT=# 2.350 951127487023154944 104.47553479331 +41.43797031725 13.3519 12.8956 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.350#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118282_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118282_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:01:02.40 +40:52:34.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 3.935 950901984059456768 105.26131619615 +40.87681310230 13.4487 12.7636 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.935#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118283_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118283_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118286_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118286_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:01:14.99 +40:41:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.98, MAG_FAINT_SEARCH_LIMIT=14.96)GAIADR2_OUTPUT=# 3.824 950847111557291136 105.31109218753 +40.69587386751 13.5469 13.0530 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.824#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118291_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118291_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:16:12.02 +33:29:11.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.06, MAG_FAINT_SEARCH_LIMIT=15.04)GAIADR2_OUTPUT=# 0.699 896309067077257728 109.04997980776 +33.48672957311 13.9611 13.4867 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.699#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118292_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118292_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:00:22.70 +41:51:07.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.95, MAG_FAINT_SEARCH_LIMIT=14.93)GAIADR2_OUTPUT=# 3.459 951165626332759680 105.09332986876 +41.85225461953 13.4805 13.0032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.459#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118295_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118295_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:01:15.51 +41:51:55.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.88, MAG_FAINT_SEARCH_LIMIT=14.86)GAIADR2_OUTPUT=# 4.992 951152122955432320 105.31286792812 +41.86579212729 13.5178 13.0995 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.992#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118299_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118299_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
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Considering the candidate 118304_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118304_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:06:50.84 +35:52:31.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.26, MAG_FAINT_SEARCH_LIMIT=15.24)GAIADR2_OUTPUT=# 1.666 945761767199772160 106.71167222112 +35.87591607369 14.2776 13.7335 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.666#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118305_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118305_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 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 118311_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118311_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 06:59:37.71 +41:39:55.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.10, MAG_FAINT_SEARCH_LIMIT=15.08)GAIADR2_OUTPUT=# 4.131 951157066461396736 104.90861529096 +41.66569484354 13.0934 12.4310 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.131#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118313_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118313_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118322_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118322_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118329_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118329_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118332_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118332_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 118333_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118333_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118336_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118336_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118349_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118349_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 06:58:56.67 +39:05:47.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.71, MAG_FAINT_SEARCH_LIMIT=14.69)GAIADR2_OUTPUT=# 5.488 947289641685972992 104.73417202670 +39.09642099206 12.8911 12.1886 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.488#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118352_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118352_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:00:12.67 +42:05:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.75, MAG_FAINT_SEARCH_LIMIT=14.73)GAIADR2_OUTPUT=# 5.845 951169818220694784 105.05494595548 +42.08842268936 12.8416 12.1408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.845#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118353_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118353_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118354_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118354_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 118355_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118355_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:00:43.67 +40:09:23.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 3.670 950448912253070848 105.18323359895 +40.15693801167 13.1060 12.6256 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.670#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118357_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118357_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:03:41.78 +41:53:11.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.48, MAG_FAINT_SEARCH_LIMIT=14.46)GAIADR2_OUTPUT=# 3.916 951050108891555968 105.92549698555 +41.88671980571 13.0004 12.4932 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.916#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118359_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118359_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118361_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118361_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118363_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118363_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:01:54.20 +42:50:13.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118365_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118365_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:00:14.42 +42:06:01.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118366_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118366_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:51:54.17 +37:15:22.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.148 919067205425325312 117.97550514605 +37.25658043326 13.4069 12.9105 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118367_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118367_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118368_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118368_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:26:04.29 +39:44:16.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 0.869 900085133603579904 111.51818689625 +39.73788840950 13.3546 12.9198 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.869#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118373_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118373_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118381_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118381_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 118384_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118384_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118385_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118385_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:28:16.07 +33:29:25.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118386_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118386_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118397_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118397_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 06:58:36.22 +41:19:18.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118405_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118405_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:00:09.82 +38:41:16.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.05, MAG_FAINT_SEARCH_LIMIT=14.03)GAIADR2_OUTPUT=# 2.598 947219169862704768 105.04003497283 +38.68772686333 12.5805 11.9761 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.598#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118408_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118408_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 06:57:50.69 +41:30:30.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.14, MAG_FAINT_SEARCH_LIMIT=14.12)GAIADR2_OUTPUT=# 5.438 951175070963747072 104.46316247494 +41.50881931578 12.1391 11.4124 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.438#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118409_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118409_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:28:23.79 +33:12:44.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.12, MAG_FAINT_SEARCH_LIMIT=14.10)GAIADR2_OUTPUT=# 0.731 893473044335445248 112.09928330027 +33.21237597367 13.2023 12.7538 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.731#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118411_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118411_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:30:05.39 +35:19:20.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.06, MAG_FAINT_SEARCH_LIMIT=14.04)GAIADR2_OUTPUT=# 1.485 893944017565848192 112.52240975714 +35.32288278486 13.1310 12.7351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.485#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118414_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118414_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 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 118415_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118415_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:00:52.31 +40:48:29.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 4.298 950895868025947392 105.21951444217 +40.80827775869 12.2482 11.5816 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.298#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118416_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118416_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118421_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118421_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:00:21.72 +41:58:28.6 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=12.89, MAG_FAINT_SEARCH_LIMIT=13.87)
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Considering the candidate 118426_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118426_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:25:31.94 +32:59:13.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.87, MAG_FAINT_SEARCH_LIMIT=13.85)GAIADR2_OUTPUT=# 1.516 893081450693880704 111.38355839813 +32.98710858738 12.9615 12.4842 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.516#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118429_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118429_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118432_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118432_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118433_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118433_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118437_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118437_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118439_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118439_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:16:34.90 +38:18:24.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 1.952 946473529180066688 109.14565527474 +38.30731456910 12.8195 12.4255 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.952#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118440_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118440_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118445_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118445_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:19:35.76 +34:28:21.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118446_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118446_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118447_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118447_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
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Considering the candidate 118455_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118455_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 06:58:37.51 +40:31:52.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.72, MAG_FAINT_SEARCH_LIMIT=12.70)GAIADR2_OUTPUT=# 3.344 950524198735921024 104.65750690397 +40.53101239395 11.1524 10.4734 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.344#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118456_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118456_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:02:35.42 +42:48:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.71, MAG_FAINT_SEARCH_LIMIT=12.69)GAIADR2_OUTPUT=# 2.919 952796305155735936 105.64867737939 +42.81069919569 11.1011 10.3576 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.919#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118458_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118458_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:02:10.55 +42:41:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.50, MAG_FAINT_SEARCH_LIMIT=12.48)GAIADR2_OUTPUT=# 4.241 951295845444097280 105.54555716316 +42.68514102145 10.8327 10.1264 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.241#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118460_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118460_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:01:46.15 +42:15:54.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 2.392 951257676072046080 105.44311376217 +42.26548902951 10.5214 9.7864 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.392#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118461_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118461_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 06:59:08.77 +42:34:07.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.17, MAG_FAINT_SEARCH_LIMIT=12.15)GAIADR2_OUTPUT=# 4.015 951328491492765824 104.78506605757 +42.56908378749 10.5102 9.8721 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.015#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118462_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118462_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:01:33.43 +42:49:56.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.38, MAG_FAINT_SEARCH_LIMIT=11.36)GAIADR2_OUTPUT=# 3.975 952810457071096576 105.39079708100 +42.83232053389 9.7117 9.0219 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.975#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118489_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118489_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 08:01:58.04 +34:06:22.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118498_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118498_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 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 118516_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118516_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 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 118529_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118529_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:49:42.07 +38:02:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.21, MAG_FAINT_SEARCH_LIMIT=13.19)GAIADR2_OUTPUT=# 1.110 920002614942859776 117.42512586460 +38.03377938133 12.2272 11.6243 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.110#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
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Considering the candidate 118541_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118541_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 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 118583_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118583_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 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 118604_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118604_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 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 118606_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118606_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 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 118635_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118635_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 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 118642_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118642_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 08:07:53.17 +38:35:53.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118664_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118664_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:05:55.51 +33:43:21.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118666_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118666_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:15:33.86 +42:05:02.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118681_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118681_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:23:15.81 +35:10:43.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118684_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118684_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 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 118702_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118702_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118706_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118706_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118737_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118737_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:17:44.01 +34:07:15.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118750_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118750_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:21:01.85 +35:19:16.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 118751_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118751_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:06:07.60 +34:26:30.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 118770_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118770_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:11:15.34 +33:05:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.85, MAG_FAINT_SEARCH_LIMIT=14.83)GAIADR2_OUTPUT=# 1.382 890422178743511168 107.81384752153 +33.09856506345 13.9724 13.4809 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.382#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118781_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118781_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:42:50.12 +33:24:30.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118782_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118782_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:22:23.71 +33:10:47.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.94, MAG_FAINT_SEARCH_LIMIT=14.92)GAIADR2_OUTPUT=# 1.242 893238234180033664 110.59876538202 +33.18020529446 14.0086 13.3558 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.242#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118790_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118790_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118840_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118840_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118859_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118859_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:34:56.93 +35:45:56.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118882_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118882_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:05:28.91 +42:21:45.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.17, MAG_FAINT_SEARCH_LIMIT=15.15)GAIADR2_OUTPUT=# 2.300 952537537669252992 106.37006796682 +42.36332000795 13.8206 13.1247 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.300#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118891_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118891_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:11:56.57 +35:10:28.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.21, MAG_FAINT_SEARCH_LIMIT=15.19)GAIADR2_OUTPUT=# 1.041 897443178962091776 107.98546771893 +35.17442674097 14.2069 13.5621 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.041#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118920_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118920_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:05:58.23 +39:52:35.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.13, MAG_FAINT_SEARCH_LIMIT=15.11)GAIADR2_OUTPUT=# 1.791 947761710131110400 106.49263125124 +39.87691416566 14.1176 13.7703 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.791#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118945_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118945_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118959_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
Preparing report for the candidate 118959_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118964_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118964_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 118980_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 118980_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:13:17.64 +33:19:27.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.42, MAG_FAINT_SEARCH_LIMIT=15.40)GAIADR2_OUTPUT=# 1.240 890475883014752896 108.32308870771 +33.32439416072 14.2564 13.5774 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119011_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 119011_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:33:55.35 +43:03:52.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.46, MAG_FAINT_SEARCH_LIMIT=15.44)GAIADR2_OUTPUT=# 2.161 924906642961299712 113.48099235909 +43.06517569034 14.0898 13.0863 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.161#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119012_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 119012_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:13:00.87 +36:47:34.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 1.554 897890538459057792 108.25309162970 +36.79289555631 14.4156 13.7032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.554#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119015_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 119015_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
Rejecting candidate due to large distance (23.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119016_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 119016_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:44:21.66 +33:13:23.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.45, MAG_FAINT_SEARCH_LIMIT=15.43)GAIADR2_OUTPUT=# 2.754 881981983890876416 116.09057915355 +33.22248067351 14.5055 14.0674 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.754#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119027_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 119027_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:16:19.52 +34:26:40.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.49, MAG_FAINT_SEARCH_LIMIT=15.47)GAIADR2_OUTPUT=# 0.726 896607309606780160 109.08150773583 +34.44441401120 15.1330 14.6155 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.726#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119070_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 119070_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 08:15:27.31 +41:55:30.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.47, MAG_FAINT_SEARCH_LIMIT=15.45)GAIADR2_OUTPUT=# 2.826 915734173364175232 123.86274701335 +41.92516531378 14.7376 14.0685 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.826#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 119071_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 119071_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 08:04:45.52 +39:45:29.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=14.44, MAG_FAINT_SEARCH_LIMIT=15.42)GAIADR2_OUTPUT=# 0.761 921102745045437184 121.18994103581 +39.75804082846 14.5001 13.8773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.761#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.9#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02993_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 02993_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 64977_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123
The candidate 64977_fd_Lyn-05-Q2b1x1_2026-03-19_22-51-32_20.00sec_-15.00C_LIGHT_0123 did not pass the final checks
**** FOUND 07:26:13.74 +33:22:24.6 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 5s
make_report_in_HTML.sh TOTAL: 68s
Prepared the HTML report for the field Lyn-05-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
07:04:36.70 +41:40:51.8
06:58:11.32 +40:07:46.1
07:00:13.58 +41:12:19.6
07:01:47.41 +42:48:16.0
07:00:13.65 +41:34:38.5
06:59:08.44 +42:16:19.2
06:59:57.13 +41:44:16.9
06:59:24.84 +42:36:47.3
06:59:14.44 +42:28:19.1
06:59:34.31 +42:23:12.6
06:58:37.72 +40:53:59.4
06:57:33.47 +42:20:05.3
06:58:50.06 +41:17:45.8
06:57:37.51 +41:45:12.2
07:01:02.91 +42:29:41.3
06:57:57.84 +41:00:03.5
06:58:21.61 +41:26:07.1
07:01:08.31 +42:16:54.5
07:00:34.89 +42:41:04.2
07:00:00.28 +42:27:21.9
06:57:50.26 +42:33:23.0
07:02:00.21 +42:51:49.2
07:04:56.75 +42:43:47.4
06:57:03.90 +42:41:58.5
07:26:37.51 +36:50:59.2
07:59:08.87 +33:11:12.1
07:44:51.90 +34:34:38.9
########### Completed Lyn-05-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 ####
07:04:36.70 +41:40:51.8
06:58:11.32 +40:07:46.1
07:00:13.58 +41:12:19.6
07:01:47.41 +42:48:16.0
07:00:13.65 +41:34:38.5
06:59:08.44 +42:16:19.2
06:59:57.13 +41:44:16.9
06:59:24.84 +42:36:47.3
06:59:14.44 +42:28:19.1
06:59:34.31 +42:23:12.6
06:58:37.72 +40:53:59.4
06:57:33.47 +42:20:05.3
06:58:50.06 +41:17:45.8
06:57:37.51 +41:45:12.2
07:01:02.91 +42:29:41.3
06:57:57.84 +41:00:03.5
06:58:21.61 +41:26:07.1
07:01:08.31 +42:16:54.5
07:00:34.89 +42:41:04.2
07:00:00.28 +42:27:21.9
06:57:50.26 +42:33:23.0
07:02:00.21 +42:51:49.2
07:04:56.75 +42:43:47.4
06:57:03.90 +42:41:58.5
07:26:37.51 +36:50:59.2
07:59:08.87 +33:11:12.1
07:44:51.90 +34:34:38.9
###################################################################################
07:04:36.70 +41:40:51.8 -- not an asteroid (will add it to exclusion list)
06:58:11.32 +40:07:46.1 -- not an asteroid (will add it to exclusion list)
07:00:13.58 +41:12:19.6 -- not an asteroid (will add it to exclusion list)
07:01:47.41 +42:48:16.0 -- not an asteroid (will add it to exclusion list)
07:00:13.65 +41:34:38.5 -- not an asteroid (will add it to exclusion list)
06:59:08.44 +42:16:19.2 -- not an asteroid (will add it to exclusion list)
06:59:57.13 +41:44:16.9 -- not an asteroid (will add it to exclusion list)
06:59:24.84 +42:36:47.3 -- not an asteroid (will add it to exclusion list)
06:59:14.44 +42:28:19.1 -- not an asteroid (will add it to exclusion list)
06:59:34.31 +42:23:12.6 -- not an asteroid (will add it to exclusion list)
06:58:37.72 +40:53:59.4 -- not an asteroid (will add it to exclusion list)
06:57:33.47 +42:20:05.3 -- not an asteroid (will add it to exclusion list)
06:58:50.06 +41:17:45.8 -- not an asteroid (will add it to exclusion list)
06:57:37.51 +41:45:12.2 -- not an asteroid (will add it to exclusion list)
07:01:02.91 +42:29:41.3 -- not an asteroid (will add it to exclusion list)
06:57:57.84 +41:00:03.5 -- not an asteroid (will add it to exclusion list)
06:58:21.61 +41:26:07.1 -- not an asteroid (will add it to exclusion list)
07:01:08.31 +42:16:54.5 -- not an asteroid (will add it to exclusion list)
07:00:34.89 +42:41:04.2 -- not an asteroid (will add it to exclusion list)
07:00:00.28 +42:27:21.9 -- not an asteroid (will add it to exclusion list)
06:57:50.26 +42:33:23.0 -- not an asteroid (will add it to exclusion list)
07:02:00.21 +42:51:49.2 -- not an asteroid (will add it to exclusion list)
07:04:56.75 +42:43:47.4 -- not an asteroid (will add it to exclusion list)
06:57:03.90 +42:41:58.5 -- not an asteroid (will add it to exclusion list)
07:26:37.51 +36:50:59.2 -- asteroid (will NOT add it to exclusion list)
07:59:08.87 +33:11:12.1 -- not an asteroid (will add it to exclusion list)
07:44:51.90 +34:34:38.9 -- asteroid (will NOT add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
06:57:03.90 +42:41:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:33.47 +42:20:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:37.51 +41:45:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:50.26 +42:33:23.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:57:57.84 +41:00:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:11.32 +40:07:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:21.61 +41:26:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:37.72 +40:53:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:58:50.06 +41:17:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:08.44 +42:16:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:14.44 +42:28:19.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:24.84 +42:36:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:34.31 +42:23:12.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:59:57.13 +41:44:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:00.28 +42:27:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:13.58 +41:12:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:13.65 +41:34:38.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:00:34.89 +42:41:04.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:02.91 +42:29:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:08.31 +42:16:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
07:01:47.41 +42:48:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
07:02:00.21 +42:51:49.2 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:36.70 +41:40:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:04:56.75 +42:43:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
07:59:08.87 +33:11:12.1 -- 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)
06:57:03.90 +42:41:58.5 -- not a known variable star
06:57:33.47 +42:20:05.3 -- not a known variable star
06:57:37.51 +41:45:12.2 -- a known variable star
06:57:50.26 +42:33:23.0 -- not a known variable star
06:57:57.84 +41:00:03.5 -- not a known variable star
06:58:11.32 +40:07:46.1 -- not a known variable star
06:58:21.61 +41:26:07.1 -- not a known variable star
06:58:37.72 +40:53:59.4 -- not a known variable star
06:58:50.06 +41:17:45.8 -- not a known variable star
06:59:08.44 +42:16:19.2 -- not a known variable star
06:59:14.44 +42:28:19.1 -- not a known variable star
06:59:24.84 +42:36:47.3 -- not a known variable star
06:59:34.31 +42:23:12.6 -- not a known variable star
06:59:57.13 +41:44:16.9 -- not a known variable star
07:00:00.28 +42:27:21.9 -- not a known variable star
07:00:13.58 +41:12:19.6 -- a known variable star
07:00:13.65 +41:34:38.5 -- not a known variable star
07:00:34.89 +42:41:04.2 -- not a known variable star
07:01:02.91 +42:29:41.3 -- not a known variable star
07:01:08.31 +42:16:54.5 -- not a known variable star
07:01:47.41 +42:48:16.0 -- not a known variable star
07:02:00.21 +42:51:49.2 -- not a known variable star
07:04:36.70 +41:40:51.8 -- not a known variable star
07:04:56.75 +42:43:47.4 -- not a known variable star
07:59:08.87 +33:11:12.1 -- not a known variable star
Found 23 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
25 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
Adding identified Gaia sources from exclusion_list_gaiadr2.txt
Adding identified Gaia sources from exclusion_list_apass.txt
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
06:57:03.90 +42:41:58.5
06:57:33.47 +42:20:05.3
06:57:37.51 +41:45:12.2
06:57:50.26 +42:33:23.0
06:57:57.84 +41:00:03.5
06:58:11.32 +40:07:46.1
06:58:21.61 +41:26:07.1
06:58:37.72 +40:53:59.4
06:58:50.06 +41:17:45.8
06:59:08.44 +42:16:19.2
06:59:14.44 +42:28:19.1
06:59:24.84 +42:36:47.3
06:59:34.31 +42:23:12.6
06:59:57.13 +41:44:16.9
07:00:00.28 +42:27:21.9
07:00:13.58 +41:12:19.6
07:00:13.65 +41:34:38.5
07:00:34.89 +42:41:04.2
07:01:02.91 +42:29:41.3
07:01:08.31 +42:16:54.5
07:01:47.41 +42:48:16.0
07:02:00.21 +42:51:49.2
07:04:36.70 +41:40:51.8
07:04:56.75 +42:43:47.4
07:59:08.87 +33:11:12.1
07:37:58.99 +38:15:21.8
08:15:59.30 +40:33:02.0
07:44:34.49 +36:39:10.7
07:48:01.95 +35:33:35.1
07:30:59.14 +40:46:59.2
07:30:03.30 +40:06:40.1
07:40:48.15 +38:01:06.0
07:42:27.90 +38:02:41.9
07:46:58.23 +41:40:30.5
07:03:34.59 +41:55:12.7
07:02:41.84 +42:28:01.8
07:20:50.64 +39:07:25.0
07:01:18.81 +33:25:19.1
07:00:40.98 +40:45:04.0
07:30:22.66 +42:21:20.5
07:11:41.34 +42:43:52.3
07:03:09.38 +41:45:03.2
07:07:11.40 +42:27:54.9
06:59:48.53 +42:33:04.7
07:01:38.68 +42:22:07.6
07:18:55.73 +33:56:27.3
06:58:35.24 +40:13:38.7
07:00:23.87 +42:00:33.5
07:00:13.15 +39:24:51.6
07:01:35.40 +41:19:06.7
06:57:53.96 +41:26:15.3
07:01:02.40 +40:52:34.9
07:01:14.99 +40:41:44.3
07:16:12.02 +33:29:11.6
07:00:22.70 +41:51:07.3
07:01:15.51 +41:51:55.2
07:06:50.84 +35:52:31.7
06:59:37.71 +41:39:55.5
06:58:56.67 +39:05:47.7
07:00:12.67 +42:05:17.3
07:00:43.67 +40:09:23.9
07:03:41.78 +41:53:11.2
07:51:54.17 +37:15:22.7
07:26:04.29 +39:44:16.5
07:00:09.82 +38:41:16.6
06:57:50.69 +41:30:30.4
07:28:23.79 +33:12:44.0
07:30:05.39 +35:19:20.9
07:00:52.31 +40:48:29.1
07:25:31.94 +32:59:13.1
07:16:34.90 +38:18:24.5
06:58:37.51 +40:31:52.0
07:02:35.42 +42:48:38.1
07:02:10.55 +42:41:06.8
07:01:46.15 +42:15:54.8
06:59:08.77 +42:34:07.8
07:01:33.43 +42:49:56.3
07:49:42.07 +38:02:00.6
07:11:15.34 +33:05:56.2
07:22:23.71 +33:10:47.5
07:05:28.91 +42:21:45.9
07:11:56.57 +35:10:28.7
07:05:58.23 +39:52:35.1
07:13:17.64 +33:19:27.9
07:33:55.35 +43:03:52.7
07:13:00.87 +36:47:34.2
07:44:21.66 +33:13:23.5
07:16:19.52 +34:26:40.4
08:15:27.31 +41:55:30.2
08:04:45.52 +39:45:29.0
07:00:21.72 +41:58:28.6
####################################################
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461119.66037281 -observatory 500
22:37:27.37 -07:27:01.9 Mercury (1.1mag)
01:02:45.37 +05:43:33.4 Venus (-3.9mag)
23:00:42.87 -07:29:40.1 Mars (1.2mag)
07:04:39.13 +22:58:08.5 Jupiter (-2.3mag)
00:16:57.88 -00:28:39.6 Saturn (0.9mag)
03:42:48.58 +19:31:27.1 Uranus (5.8mag)
00:07:10.38 -00:38:47.4 Neptune (7.8mag)
20:31:55.80 -22:53:54.6 Pluto (14.5mag)
00:45:29.56 +08:09:45.5 Moon (-8.4mag)
-rw-r--r-- 1 apache apache 361 Mar 19 23:11 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461119.66037281:
07:04:30.44 +22:58:25.2 Io (5.6mag)
07:04:40.41 +22:58:02.3 Europa (5.7mag)
07:04:28.56 +22:58:20.8 Ganymede (5.2mag)
07:04:09.98 +22:58:54.4 Callisto (6.4mag)
07:08:40.56 +23:00:14.9 Himalia (15.2mag)
07:04:35.50 +22:58:13.1 Thebe (16.0mag)
07:08:14.40 +23:23:09.0 Elara (17.1mag)
07:01:43.88 +23:52:16.3 Pasiphae (17.2mag)
07:13:27.23 +22:52:26.6 Carme (18.3mag)
00:16:49.79 -00:28:29.0 Titan (8.8mag)
00:16:57.46 -00:28:34.8 Rhea (10.1mag)
00:17:28.26 -00:26:40.9 Iapetus (11.5mag)
00:17:12.06 -00:28:47.9 Hyperion (14.8mag)
00:18:52.46 -00:17:19.4 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 19 23:11 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461119.66037281:
12:42:50.02 +09:44:26.7 JWST
19:33:23.37 +08:17:55.8 Chandra
16:12:34.23 -54:05:44.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 19 23:11 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461119.66037281 -observatory 500
18:34:41.69 -27:25:29.5 14.1mag P/2010 H2 (Vales)
04:50:46.64 -71:04:53.0 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:28:41.08 +31:17:41.8 17.0mag C/2017 K2 (PANSTARRS)
17:29:29.66 +07:18:15.0 17.6mag C/2021 G2 (ATLAS)
23:01:13.78 +28:25:12.5 16.9mag C/2022 E2 (ATLAS)
03:59:37.80 +25:16:12.1 15.7mag C/2022 N2 (PANSTARRS)
09:01:58.38 +31:24:54.5 16.0mag C/2022 QE78 (ATLAS)
08:30:16.19 -03:16:55.1 17.2mag C/2022 R6 (PANSTARRS)
18:56:28.37 +16:13:11.5 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:46:26.27 -11:51:11.3 17.6mag P/2023 B1 (PANSTARRS)
09:25:14.20 -16:28:33.4 17.4mag C/2023 F3 (ATLAS)
21:20:26.16 +61:40:09.7 17.4mag C/2023 H5 (Lemmon)
19:33:24.52 -03:31:04.6 14.5mag C/2023 R1 (PANSTARRS)
21:35:38.06 +82:46:46.7 17.7mag C/2023 X2 (Lemmon)
06:15:41.35 +63:47:50.1 16.8mag C/2024 A1 (ATLAS)
04:03:41.29 +04:34:17.8 9.0mag C/2024 E1 (Wierzchos)
11:23:20.05 +02:33:51.7 18.0mag C/2024 G2 (ATLAS)
16:32:33.75 +02:01:59.5 17.5mag C/2024 G6 (ATLAS)
20:09:36.56 +08:34:23.7 14.9mag C/2024 J3 (ATLAS)
03:04:04.17 -26:48:03.4 16.5mag C/2024 T5 (ATLAS)
04:57:03.18 +52:52:28.0 17.6mag C/2025 J1 (Borisov)
15:16:00.88 +16:19:55.6 14.4mag C/2025 L1 (ATLAS)
02:47:29.06 -22:28:16.4 17.6mag C/2025 Q3 (ATLAS)
22:32:22.55 +18:57:27.6 12.6mag C/2025 R3 (PANSTARRS)
13:05:23.06 +01:15:22.9 17.7mag C/2025 Y1 (ATLAS)
02:11:50.46 -06:51:53.9 14.3mag C/2026 A1 (MAPS)
22:36:04.98 +30:47:20.8 13.7mag C/2026 B2 (Sun-Gao)
17:50:25.71 -10:51:54.0 13.4mag 10P/Tempel
15:27:10.45 +05:10:46.6 11.7mag 24P/Schaumasse
11:12:21.05 -02:30:48.4 15.6mag 29P/Schwassmann-Wachmann
17:42:47.52 -10:40:38.4 17.3mag 40P/Vaisala
10:45:35.70 -06:39:09.2 16.4mag 43P/Wolf-Harrington
01:07:41.81 +12:46:18.9 17.0mag 47P/Ashbrook-Jackson
06:27:28.16 +42:30:54.8 17.1mag 63P/Wild
22:53:01.12 -14:51:11.3 15.7mag 65P/Gunn
02:56:31.49 +10:58:19.7 15.9mag 76P/West-Kohoutek-Ikemura
00:07:45.07 +02:52:53.1 14.7mag 78P/Gehrels
21:35:50.52 -16:57:33.2 14.5mag 88P/Howell
00:58:38.60 +12:58:34.7 15.3mag 93P/Lovas
04:09:20.91 +30:37:44.2 16.5mag 123P/West-Hartley
08:07:34.20 +50:38:18.8 16.2mag 124P/Mrkos
01:53:07.85 +11:15:15.1 16.4mag 128P/Shoemaker-Holt
01:55:48.82 +10:54:47.1 17.4mag 131P/Mueller
23:16:25.45 +02:45:47.9 13.1mag 141P/Machholz
23:26:29.63 -04:41:55.6 13.1mag 141P-A/Machholz
22:27:47.40 -07:11:02.1 16.2mag 141P-D/Machholz
23:48:04.74 -14:32:00.1 15.5mag 162P/SidingSpring
10:39:56.53 +32:02:13.7 17.5mag 164P/Christensen
05:48:17.63 +24:44:27.2 17.5mag 198P/ODAS
15:34:24.44 -03:29:21.0 16.9mag 210P/Christensen
20:08:36.24 -17:43:28.7 17.1mag 218P/LINEAR
16:58:22.33 -16:44:50.7 16.3mag 235P/LINEAR
04:39:51.34 +31:53:16.8 16.3mag 240P/NEAT
07:29:45.44 -08:29:17.0 17.5mag 242P/Spahr
15:48:36.77 +05:02:30.2 17.7mag 391P/Kowalski
07:27:55.71 +21:05:34.6 17.5mag 450P/LONEOS
04:59:57.16 +46:40:19.8 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 19 23:11 comets.txt
############################################################
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 23:11 asassn_transients_list.txt
############################################################
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 23:11 tocp_transients_list.txt