This analysis is done by the script util/transients/transient_factory_test31.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48
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 01 18.3133 2461058.8133 12.23 08:06:56.89 +58:08:08.2
159.31347 32.63466 galactic Lyn Second-epoch detections are separated by 7.2" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:06:56.89 +58:08:08.2 (user input) | T | P | (position from user input) SpType: G0 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461058.8133,12.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 12.23CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:06:56.89 +58:08:08.2 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,11.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 11.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:25:58.06 +56:46:12.0 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3133 2461058.8133 11.99 08:05:36.82 +56:18:39.4
161.47609 32.43935 galactic Lyn Second-epoch detections are separated by 4.8" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:05:36.82 +56:18:39.4 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461058.8133,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 11.99CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:05:36.82 +56:18:39.4 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,12.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 12.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:08:59.64 +49:19:00.6 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 12.12CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:31:49.31 +52:25:34.3 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3133 2461058.8133 12.35 08:42:32.62 +53:55:56.7
164.16669 37.78967 galactic UMa Second-epoch detections are separated by 5.9" and 5.0 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 1030351526051764096 | 08:42:29.55 +53:56:16.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G9 (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!
TCP 2026 01 18.3133* 08 42 32.62 +53 55 56.7 12.3 U UMa 9 0
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 1030351526051764096,2461058.8133,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 1030351526051764096 20260118.3133 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:42:32.62 +53:55:56.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3133 2461058.8133 12.35 08:49:43.70 +54:24:08.5
163.43563 38.78827 galactic UMa Second-epoch detections are separated by 6.3" and 5.0 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 1029976760088920192 | 08:49:42.82 +54:24:22.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 (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!
TCP 2026 01 18.3133* 08 49 43.70 +54 24 08.5 12.3 U UMa 9 0
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 1029976760088920192,2461058.8133,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 1029976760088920192 20260118.3133 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:49:43.70 +54:24:08.5 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,13.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 13.86CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:41:03.43 +50:16:47.2 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:41:54.17 +57:25:41.2 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:21:12.99 +54:14:46.9 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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!
TCP 2026 01 18.3133* 08 54 41.85 +53 52 35.1 13.4 U UMa 9 0
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,2461058.8133,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:54:41.85 +53:52:35.1 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:47:12.64 +55:41:35.3 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3133 2461058.8133 13.06 07:37:53.81 +53:43:47.0
164.07649 28.27037 galactic Lyn Second-epoch detections are separated by 7.7" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 07:37:53.81 +53:43:47.0 (user input) | T | P | (position from user input) SpType: K5 (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,2461058.8133,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:37:53.81 +53:43:47.0 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 12.70CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:45:07.66 +55:10:47.4 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:11:34.32 +56:27:13.8 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:50:37.68 +51:01:31.4 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:43:46.59 +52:22:38.2 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3133 2461058.8133 12.46 09:10:38.26 +56:19:00.2
160.30440 41.38602 galactic UMa Second-epoch detections are separated by 6.1" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1024418286430182528 | 09:10:40.43 +56:19:09.1 (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!
TCP 2026 01 18.3133* 09 10 38.26 +56 19 00.2 12.5 U UMa 9 0
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 1024418286430182528,2461058.8133,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 1024418286430182528 20260118.3133 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:38.26 +56:19:00.2 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 12.90CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:49:30.30 +53:05:51.0 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 12.92CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:53:00.22 +55:01:13.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 13.28CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:59:23.05 +51:15:49.2 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:51:42.10 +51:51:21.0 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:33:38.71 +58:26:22.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:43:08.85 +49:08:30.4 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:39:13.81 +56:07:20.5 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3133 2461058.8133 13.71 08:48:51.88 +52:46:47.9
165.52348 38.83088 galactic UMa Second-epoch detections are separated by 7.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1029295067176349312 | 08:48:47.77 +52:46:37.9 (Gaia DR3) | VAR (local) | G (local) | Gaia3var=VARIABLE
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!
TCP 2026 01 18.3133* 08 48 51.88 +52 46 47.9 13.7 U UMa 9 0
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 1029295067176349312,2461058.8133,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 1029295067176349312 20260118.3133 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:48:51.88 +52:46:47.9 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 13.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:43:18.77 +50:15:19.5 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,13.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 13.95CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:39:19.49 +57:31:40.9 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,13.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 13.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:46:18.41 +52:12:40.5 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:41:54.05 +50:44:01.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,14.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 14.08CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:53:17.72 +53:23:32.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,13.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:43:14.18 +52:05:47.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 13.89CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:45:11.12 +52:33:14.0 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:54:10.88 +50:47:34.4 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,14.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 14.00CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:51:02.32 +52:37:18.4 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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!
TCP 2026 01 18.3133* 09 18 15.89 +57 55 42.8 14.0 U UMa 9 0
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,2461058.8133,13.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:18:15.89 +57:55:42.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_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,2461058.8133,13.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:37:36.95 +56:27:12.5 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 01 18.3133 2461058.8133 11.16 08:05:36.93 +56:18:47.6
161.47339 32.43965 galactic Lyn Second-epoch detections are separated by 6.7" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 08:05:36.93 +56:18:47.6 (user input) | T | P | (position from user input) SpType: F5 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461058.8133,11.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 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 20260118.3133 11.16CV 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 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:05:36.93 +56:18:47.6 ;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-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20_00sec_-15_00C_LIGHT_0319_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20_00sec_-15_00C_LIGHT_0318_fits__*pix.png animation_v2.gif
Processing complete!
Total number of candidates identified: 38
Processing log:
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.94487828 23.12.2025 10:40:27.483 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
First image: 2461032.94487828 23.12.2025 10:40:27.483 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
Last image: 2461058.81350709 18.01.2026 07:31:17.013 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 8
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.42
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: 24 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): 11030
Objects passed selection criteria: 11027
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: 10752.8
Average stars matched: 10504 (97.6866 %)
Memory usage VmPeak: 113160 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Jan 14 09:05:05 CST 2026
VaST build number 1.0rc88-183-g45c3f81a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-01-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jan 18 02:08:03 CST 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: 2461032.94487828 23.12.2025 10:40:27.483 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
First image: 2461032.94487828 23.12.2025 10:40:27.483 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
Last image: 2461058.81350709 18.01.2026 07:31:17.013 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 128
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.18
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: 139 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 2.1 # or , in mag.arcsec-2
ANALYSIS_THRESH 2.1 # or , in mag.arcsec-2
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): 63244
Objects passed selection criteria: 63070
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: 61484.2
Average stars matched: 59400.2 (96.6105 %)
Memory usage VmPeak: 163116 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Jan 14 09:05:05 CST 2026
VaST build number 1.0rc88-183-g45c3f81a
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-01-14)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Jan 18 02:27:07 CST 2026
Host name: tau
############################################################
Filtering log:
######## Processing parameters ########
AAVSO_COMMENT_STRING= NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
ASTCHECK_ASTEROID_SEARCH_RADIUS_ARCSEC=
BAD_REGION_FILE= /var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst
CAMERA_SETTINGS= TTUQ1b1x1
CHECK_POINTING_ACCURACY= yes
DARK_FRAMES_DIR= /var/www/nmw_calibration/TTUQ1b1x1/darks
EXCLUSION_LIST= ../exclusion_list_TTUQ1.txt
FILTER_BAD_IMG__MAX_APERTURE_STAR_SIZE_PIX= 12.5
FILTER_BAD_IMG__MAX_ELONGATION_AminusB_PIX= 0.55
FILTER_BAD_IMG__MIN_APERTURE_STAR_SIZE_PIX= 2.0
FILTER_BRIGHT_MAG_CUTOFF_TRANSIENT_SEARCH= -5
FILTER_FAINT_MAG_CUTOFF_TRANSIENT_SEARCH= 14.5
FLAT_FIELD_FILE= /var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit
FRAME_EDGE_OFFSET_PIX= 25
GAIA_BAND_FOR_CATALOGED_SOURCE_CHECK=
MAX_NEW_TO_REF_MEAN_IMG_VALUE_RATIO= 100
MAX_NEW_IMG_MEAN_VALUE= 25000
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS= 0.18
MAX_SD_RATIO_OF_SECOND_EPOCH_IMGS_SOFT_LIMIT= 0.12
MPC_CODE= 500
NMW_CALIBRATION= /var/www/nmw_calibration
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_HARD_LIMIT= 3000
NUMBER_OF_DETECTED_TRANSIENTS_BEFORE_FILTERING_SOFT_LIMIT= 2000
OMP_NUM_THREADS=
ONLINE_MPCHECKER_BUTTON_ASTEROID_SEARCH_RADIUS_ARCMIN=
PHOTOMETRIC_CALIBRATION=
REQUIRE_PIX_SHIFT_BETWEEN_IMAGES_FOR_TRANSIENT_CANDIDATES= yes
SEXTRACTOR_CONFIG_BRIGHTSTARPASS= default.sex.telephoto_lens_onlybrightstars_v1
SEXTRACTOR_CONFIG_FILES= default.sex.telephoto_lens_onlybrightstars_v1 default.sex.telephoto_lens_vSTL
STARMATCH_RADIUS_PIX= 3.5
SYSREM_ITERATIONS= 0
TELESCOP=
TELESCOP_NAME_KNOWN_TO_VaST_FOR_FOV_DETERMINATION=
UCAC5_PLATESOLVE_ITERATIONS= 2
FPACK_FULLY_CALIBRATED_IMAGE= no
#######################################
HOSTNAME= tau
USER=
HOME=
#######################################
Reference image directory is set to /mnt/usb2/NMW-TexasTech/reference_imgs
VIZIER_SITE=vizier.cds.unistra.fr
INFO: MAKE_PNG_PLOTS is set to yes
FITS_FILE_EXT=fits
CALIBRATION_STATUS_PREFIX=
Fields in the data directory:
Lyn-02-Q1b1x1
#######################################
########### Starting Lyn-02-Q1b1x1 ###########
Processing Lyn-02-Q1b1x1
server tau has sufficient free disk space available: 395666 MB at /mnt/usb2/NMW-TexasTech/workdir
server tau has sufficient free disk space available: 395666 MB at .
Checking input images (2 new)
REFERENCE_EPOCH__FIRST_IMAGE= /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
REFERENCE_EPOCH__SECOND_IMAGE= /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
Small preview (one of the new images):
Large previews of the second-epoch (new) images:
MAKE_PNG_PLOTS=yes
renamed 'Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png' -> 'transient_report/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits_preview.png'
Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
renamed 'Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png' -> 'transient_report/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits_preview.png'
Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Read-check the input FITS images... read-check OK
Blank image check the input FITS images... blank-image-check OK
Read date check the input FITS images... read-date-check OK
Mean value check the input FITS images... OK, at least two new images have mean values below the threshold.
----------------------------------------------
INFO: REFERENCE_EPOCH__FIRST_IMAGE_MEAN_VALUE= 478.7291
INFO: REFERENCE_EPOCH__FIRST_IMAGE_SD= 572.9351
INFO: SECOND_EPOCH__FIRST_IMAGE_MEAN_VALUE= 938.1946
INFO: SECOND_EPOCH__FIRST_IMAGE_SD= 584.0684
INFO: SECOND_EPOCH__SECOND_IMAGE_MEAN_VALUE= 939.2460
INFO: SECOND_EPOCH__SECOND_IMAGE_SD= 584.3652
----------------------------------------------
INFO: ref_to_second_epoch_img_mean_ratio= 1.95976
INFO: SECOND_EPOCH__SD_ratio= 0.001
----------------------------------------------
Calibration settings: DARK_FRAMES_DIR=/var/www/nmw_calibration/TTUQ1b1x1/darks FLAT_FIELD_FILE=/var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit
EXPTIME = 20.0 / [s] Exposure duration
SET-TEMP= -15.0 / [degC] CCD temperature setpoint
CCD-TEMP= -15.0 / [degC] CCD temperature
Exploring image header: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
CCD-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Header: 61 keys total, 10 keys left
Record 0: "" status=0
Record 1: "SIMPLE = T / C# FITS" status=0
Record 2: "BITPIX = 16" status=0
Record 3: "NAXIS = 2 / Dimensionality" status=0
Record 4: "NAXIS1 = 9576" status=0
Record 5: "NAXIS2 = 6388" status=0
Record 6: "BZERO = 32768" status=0
Record 7: "EXTEND = T / Extensions are permitted" status=0
Record 8: "IMAGETYP= 'LIGHT' / Type of exposure" status=0
Record 9: "EXPOSURE= 20.0 / [s] Exposure duration" status=0
Record 10: "EXPTIME = 20.0 / [s] Exposure duration" status=0
Record 11: "DATE-LOC= '2026-01-18T01:30:34.5200482' / Time of observation (local)" status=0
Record 12: "DATE-OBS= '2026-01-18T07:30:34.5200482' / Time of observation (UTC)" status=0
Record 13: "MJD-OBS = 61058.3128995369 / Modified Julian Date of observation" status=0
Record 14: "DATE-AVG= '2026-01-18T07:30:44.4243003' / Averaged midpoint time (UTC)" status=0
Record 15: "MJD-AVG = 61058.3130141669 / Modified Julian Date of averaged midpoint" status=0
Record 16: "XBINNING= 1 / X axis binning factor" status=0
Record 17: "YBINNING= 1 / Y axis binning factor" status=0
Record 18: "GAIN = 30 / Sensor gain" status=0
Record 19: "OFFSET = 30 / Sensor gain offset" status=0
Record 20: "XPIXSZ = 3.76 / [um] Pixel X axis size" status=0
Record 21: "YPIXSZ = 3.76 / [um] Pixel Y axis size" status=0
Record 22: "INSTRUME= 'QHY600M' / Imaging instrument name" status=0
Record 23: "CAMERAID= 'QHY600M-33d3d743814b8b447' / Imaging instrument identifier" status=0
Record 24: "SET-TEMP= -15.0 / [degC] CCD temperature setpoint" status=0
Record 25: "CCD-TEMP= -15.0 / [degC] CCD temperature" status=0
Record 26: "READOUTM= '2CMS-0' / Sensor readout mode" status=0
Record 27: "USBLIMIT= 50 / Camera-specific USB setting" status=0
Record 28: "TELESCOP= 'QHY600M-TTU1' / Name of telescope" status=0
Record 29: "FOCALLEN= 135.0 / [mm] Focal length" status=0
Record 30: "FOCRATIO= 2.2 / Focal ratio" status=0
Record 31: "RA = 127.056385483173 / [deg] RA of telescope" status=0
Record 32: "DEC = 53.9997317705712 / [deg] Declination of telescope" status=0
Record 33: "CENTALT = 69.8255555555556 / [deg] Altitude of telescope" status=0
Record 34: "CENTAZ = 358.395277777778 / [deg] Azimuth of telescope" status=0
Record 35: "AIRMASS = 1.06514783580813 / Airmass at frame center (Gueymard 1993)" status=0
Record 36: "PIERSIDE= 'East' / Telescope pointing state" status=0
Record 37: "SITEELEV= 1013.0 / [m] Observation site elevation" status=0
Record 38: "SITELAT = 33.748239 / [deg] Observation site latitude" status=0
Record 39: "SITELONG= -101.958391 / [deg] Observation site longitude" status=0
Record 40: "OBSERVER= 'Sokolovsky' / Observer name" status=0
Record 41: "OBSERVAT= 'TTU Skyview' / Observatory name" status=0
Record 42: "SITENAME= '' / Observatory site name" status=0
Record 43: "FWHEEL = 'Simulator' / Filter Wheel name" status=0
Record 44: "FILTER = 'CV' / Active filter name" status=0
Record 45: "OBJECT = 'Lyn-02' / Name of the object of interest" status=0
Record 46: "OBJCTRA = '08 28 14' / [H M S] RA of imaged object" status=0
Record 47: "OBJCTDEC= '+54 00 00' / [D M S] Declination of imaged object" status=0
Record 48: "OBJCTROT= 0.0 / [deg] planned rotation of imaged object" status=0
Record 49: "ROWORDER= 'TOP-DOWN' / FITS Image Orientation" status=0
Record 50: "EQUINOX = 2000.0 / Equinox of celestial coordinate system" status=0
Record 51: "SWCREATE= 'N.I.N.A. 3.2.0.9001 (x64)' / Software that created this file" status=0
Record 52: "QHY_EXP = 20.000096 / [s] Actual exposure time" status=0
Record 53: "QHY_PP = 13888.0 / [ps] pixelPeriod" status=0
Record 54: "QHY_LP = 85000.0 / [ns] linePeriod" status=0
Record 55: "GPS_LP = 85000.0 / [ns] linePeriod" status=0
Record 56: "QHY_FP = 20000160.0 / [us] framePeriod" status=0
Record 57: "QHY_CPL = 6120.0 / clocksPerLine" status=0
Record 58: "QHY_LPF = 235295.0 / linesPerFrame" status=0
Record 59: "QHY_AET = 20000096.0 / [us] actualExposureTime" status=0
Record 60: "QHY_LEM = T / isLongExposureMode" status=0
Record 61: "QHY_OFF0= 3767.777 / [us] RollingShutterEndOffset row 0" status=0
Allocating memory for image, dark and result arrays...
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits 9576 6388 16 bitpix
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
SET-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit
CCD-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
CCD-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit
Reading dark frame /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit 9576 6388 16 bitpix
Dark frame is subtracted, output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/d_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits :)
Spent 0.428472 seconds
renamed 'mdark_TTUQ1b1x1_-15C_20s_2026-01-08.png' -> 'transient_report/dark.png'
MegaDivider v7
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/d_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits 9576 6388 16 bitpix
Reading flat /var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit 9576 6388 16 bitpix
Avarage count on flat field image: 38918.354428
Minimal real count (from overscan): 5
Output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits :)
No overscan detected - all values seem high! (left_median=27736.5, right_median=26453.5)
renamed 'mff_TTUQ1b1x1_2025-12-22.png' -> 'transient_report/flat.png'
Using calibrated image CALIBRATED_SECOND_EPOCH__FIRST_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
EXPTIME = 20.0 / [s] Exposure duration
SET-TEMP= -15.0 / [degC] CCD temperature setpoint
CCD-TEMP= -15.0 / [degC] CCD temperature
Exploring image header: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
CCD-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Header: 61 keys total, 10 keys left
Record 0: "" status=0
Record 1: "SIMPLE = T / C# FITS" status=0
Record 2: "BITPIX = 16" status=0
Record 3: "NAXIS = 2 / Dimensionality" status=0
Record 4: "NAXIS1 = 9576" status=0
Record 5: "NAXIS2 = 6388" status=0
Record 6: "BZERO = 32768" status=0
Record 7: "EXTEND = T / Extensions are permitted" status=0
Record 8: "IMAGETYP= 'LIGHT' / Type of exposure" status=0
Record 9: "EXPOSURE= 20.0 / [s] Exposure duration" status=0
Record 10: "EXPTIME = 20.0 / [s] Exposure duration" status=0
Record 11: "DATE-LOC= '2026-01-18T01:31:17.0133345' / Time of observation (local)" status=0
Record 12: "DATE-OBS= '2026-01-18T07:31:17.0133345' / Time of observation (UTC)" status=0
Record 13: "MJD-OBS = 61058.3133913539 / Modified Julian Date of observation" status=0
Record 14: "DATE-AVG= '2026-01-18T07:31:26.9158916' / Averaged midpoint time (UTC)" status=0
Record 15: "MJD-AVG = 61058.3135059606 / Modified Julian Date of averaged midpoint" status=0
Record 16: "XBINNING= 1 / X axis binning factor" status=0
Record 17: "YBINNING= 1 / Y axis binning factor" status=0
Record 18: "GAIN = 30 / Sensor gain" status=0
Record 19: "OFFSET = 30 / Sensor gain offset" status=0
Record 20: "XPIXSZ = 3.76 / [um] Pixel X axis size" status=0
Record 21: "YPIXSZ = 3.76 / [um] Pixel Y axis size" status=0
Record 22: "INSTRUME= 'QHY600M' / Imaging instrument name" status=0
Record 23: "CAMERAID= 'QHY600M-33d3d743814b8b447' / Imaging instrument identifier" status=0
Record 24: "SET-TEMP= -15.0 / [degC] CCD temperature setpoint" status=0
Record 25: "CCD-TEMP= -15.0 / [degC] CCD temperature" status=0
Record 26: "READOUTM= '2CMS-0' / Sensor readout mode" status=0
Record 27: "USBLIMIT= 50 / Camera-specific USB setting" status=0
Record 28: "TELESCOP= 'QHY600M-TTU1' / Name of telescope" status=0
Record 29: "FOCALLEN= 135.0 / [mm] Focal length" status=0
Record 30: "FOCRATIO= 2.2 / Focal ratio" status=0
Record 31: "RA = 127.056385422832 / [deg] RA of telescope" status=0
Record 32: "DEC = 53.9997317461933 / [deg] Declination of telescope" status=0
Record 33: "CENTALT = 69.8211111111111 / [deg] Altitude of telescope" status=0
Record 34: "CENTAZ = 358.095833333333 / [deg] Azimuth of telescope" status=0
Record 35: "AIRMASS = 1.06517812836282 / Airmass at frame center (Gueymard 1993)" status=0
Record 36: "PIERSIDE= 'East' / Telescope pointing state" status=0
Record 37: "SITEELEV= 1013.0 / [m] Observation site elevation" status=0
Record 38: "SITELAT = 33.748239 / [deg] Observation site latitude" status=0
Record 39: "SITELONG= -101.958391 / [deg] Observation site longitude" status=0
Record 40: "OBSERVER= 'Sokolovsky' / Observer name" status=0
Record 41: "OBSERVAT= 'TTU Skyview' / Observatory name" status=0
Record 42: "SITENAME= '' / Observatory site name" status=0
Record 43: "FWHEEL = 'Simulator' / Filter Wheel name" status=0
Record 44: "FILTER = 'CV' / Active filter name" status=0
Record 45: "OBJECT = 'Lyn-02' / Name of the object of interest" status=0
Record 46: "OBJCTRA = '08 28 14' / [H M S] RA of imaged object" status=0
Record 47: "OBJCTDEC= '+54 00 00' / [D M S] Declination of imaged object" status=0
Record 48: "OBJCTROT= 0.0 / [deg] planned rotation of imaged object" status=0
Record 49: "ROWORDER= 'TOP-DOWN' / FITS Image Orientation" status=0
Record 50: "EQUINOX = 2000.0 / Equinox of celestial coordinate system" status=0
Record 51: "SWCREATE= 'N.I.N.A. 3.2.0.9001 (x64)' / Software that created this file" status=0
Record 52: "QHY_EXP = 20.000096 / [s] Actual exposure time" status=0
Record 53: "QHY_PP = 13888.0 / [ps] pixelPeriod" status=0
Record 54: "QHY_LP = 85000.0 / [ns] linePeriod" status=0
Record 55: "GPS_LP = 85000.0 / [ns] linePeriod" status=0
Record 56: "QHY_FP = 20000160.0 / [us] framePeriod" status=0
Record 57: "QHY_CPL = 6120.0 / clocksPerLine" status=0
Record 58: "QHY_LPF = 235295.0 / linesPerFrame" status=0
Record 59: "QHY_AET = 20000096.0 / [us] actualExposureTime" status=0
Record 60: "QHY_LEM = T / isLongExposureMode" status=0
Record 61: "QHY_OFF0= 3767.777 / [us] RollingShutterEndOffset row 0" status=0
Allocating memory for image, dark and result arrays...
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits 9576 6388 16 bitpix
SET-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
SET-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit
CCD-TEMP= -15.000000 for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
CCD-TEMP= -15.000000 for /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit
Reading dark frame /var/www/nmw_calibration/TTUQ1b1x1/darks/mdark_TTUQ1b1x1_-15C_20s_2026-01-08.fit 9576 6388 16 bitpix
Dark frame is subtracted, output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/d_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits :)
Spent 0.432626 seconds
renamed 'mdark_TTUQ1b1x1_-15C_20s_2026-01-08.png' -> 'transient_report/dark.png'
MegaDivider v7
Reading image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/d_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits 9576 6388 16 bitpix
Reading flat /var/www/nmw_calibration/TTUQ1b1x1/flats/mff_TTUQ1b1x1_2025-12-22.fit 9576 6388 16 bitpix
Avarage count on flat field image: 38918.354428
Minimal real count (from overscan): 5
Output is written to /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits :)
No overscan detected - all values seem high! (left_median=27736.5, right_median=26453.5)
renamed 'mff_TTUQ1b1x1_2025-12-22.png' -> 'transient_report/flat.png'
Using calibrated image CALIBRATED_SECOND_EPOCH__SECOND_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Dark frame used to calibrate the second-epoch images:
Flat field used to calibrate the second-epoch images:
after the calibration attempt:
SECOND_EPOCH__FIRST_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
SECOND_EPOCH__SECOND_IMAGE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Previews of the CALIBRATED second-epoch images:
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_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 --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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: 2461058.81301528
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits exists and is non-empty
Saving wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits to local_wcs_cache/
'wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits'
wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits exists and is non-empty
Saving wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits to local_wcs_cache/
'wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits' -> 'local_wcs_cache/wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits'
wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits exists and is non-empty
Saving wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits to local_wcs_cache/
'wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> 'local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits exists and is non-empty
Saving wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits to local_wcs_cache/
'wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> 'local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:28:42.230 +53:57:52.69
Second-epoch image center 08:28:35.074 +53:59:05.08
Angular distance between the image centers 0.03 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 08:28:42.230 +53:57:52.69
Second-epoch image center 08:28:37.828 +53:58:46.52
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:28:35.074 +53:59:05.08
Second-epoch second image center 08:28:37.828 +53:58:46.52
Angular distance between the image centers 0.00849 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits &> /tmp/tmp.PhF1NTXbBR
Parallel run for /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits &> /tmp/tmp.sHHYr9BzV7
Parallel run for /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits &> /tmp/tmp.FQ6Uh3blGW
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits &> /tmp/tmp.nYlNC3sKIO
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits and wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits and wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat
Found non-empty wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits and wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat
The reference image (wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits) and catalog (wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat) found
'wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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 22 out of 10919 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.789391
a=0.000000 b=1.000000 c=22.789391
From vast_summary.log: estimated ref. image limiting mag.: -7.42
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.37
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.37
____ End of magnitude calibration ____
Filter-out faint candidates...
Filter-out suspiciously bright candidates...
Filter-out candidates with large difference between measured mags in one epoch...
Filter-out small-amplitude flares...
Preparing the exclusion lists for this field
Done with filtering
Found 8 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
2.1 pix Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
2.1 pix fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
2.1 pix fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Limiting magnitude estimates:
15.4 mag. Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
15.4 mag. Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
15.3 mag. fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
15.3 mag. fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
All-image limiting magnitude estimate: 15.3 (SNR ) 12.3 (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.PhF1NTXbBR (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
verification OK: /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits has a WCS header - will blindly trust it is good...
'/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits' -> 'wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits'
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
WCS-calibrated image found: wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
Checking if the catalog wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
WCS catalog name: wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=772, passed=10919
Got 10919 stars (including 10137 good ones) from the SExtractor catalog wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat
util/solve_plate_with_UCAC5 got 10919 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.4'
Seting catalog search parameters based on the expected field of view 927.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012881 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010304 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 164 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: 11.31"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 10.40"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 216 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 10.19"
Estimated accuracy of the plate solution: 6.84"
Excluding outliers - 190 stars left (next iteration limit 149)
The image catalog is written to wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits -region wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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.sHHYr9BzV7 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
verification OK: /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits has a WCS header - will blindly trust it is good...
'/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits' -> 'wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits'
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
WCS-calibrated image found: wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
Checking if the catalog wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
WCS catalog name: wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=749, passed=10931
Got 10931 stars (including 10170 good ones) from the SExtractor catalog wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat
util/solve_plate_with_UCAC5 got 10931 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.3'
Seting catalog search parameters based on the expected field of view 927.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012879 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010303 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 165 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: 10.43"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 10.07"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 208 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.88"
Estimated accuracy of the plate solution: 7.20"
Excluding outliers - 188 stars left (next iteration limit 147)
The image catalog is written to wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits -region wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.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.FQ6Uh3blGW (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...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=756, passed=10733
Got 10733 stars (including 9964 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
util/solve_plate_with_UCAC5 got 10733 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.4'
Seting catalog search parameters based on the expected field of view 927.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012881 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010304 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 176 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: 9.72"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 9.62"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 220 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.47"
Estimated accuracy of the plate solution: 6.53"
Excluding outliers - 201 stars left (next iteration limit 152)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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.nYlNC3sKIO (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...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=792, passed=10665
Got 10665 stars (including 9862 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
util/solve_plate_with_UCAC5 got 10665 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.5'
Seting catalog search parameters based on the expected field of view 927.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012882 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010306 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 173 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: 10.04"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 9.51"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 219 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.40"
Estimated accuracy of the plate solution: 7.19"
Excluding outliers - 199 stars left (next iteration limit 152)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits'
Saving fully-calibrated image wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits' -> '/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits'
Preparing the HTML report for the field Lyn-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20649.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20661.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20663.dat to exclusion_list_local.txt
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Considering the candidate 20630_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 20630_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/20630_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/20630_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/20630_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 20632_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 20632_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/20632_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/20632_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/20632_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 20649_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 20649_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/20649_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/20649_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/20649_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 20651_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 20651_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/20651_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/20651_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/20651_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 20652_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 20652_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/20652_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/20652_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/20652_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 20656_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 20656_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
**** FOUND 08:24:49.62 +50:03:47.9 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20661_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 20661_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/20661_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/20661_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/20661_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 20663_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 20663_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/20663_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/20663_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/20663_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
Prepared the HTML report for the field Lyn-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:06:56.89 +58:08:08.2
08:25:58.06 +56:46:12.0
08:05:36.82 +56:18:39.4
08:08:59.64 +49:19:00.6
08:31:49.31 +52:25:34.3
08:42:32.62 +53:55:56.7
08:49:43.70 +54:24:08.5
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
Creating symlink local_wcs_cache/wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Creating symlink local_wcs_cache/exclusion_list_bsc.txt
Creating symlink local_wcs_cache/exclusion_list_tycho2.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-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits exists and is non-empty
wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits exists and is non-empty
wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits exists and is non-empty
wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits exists and is non-empty
The image scale is 5.81"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.7"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 08:28:42.230 +53:57:52.69
Second-epoch image center 08:28:35.074 +53:59:05.08
Angular distance between the image centers 0.03 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 08:28:42.230 +53:57:52.69
Second-epoch image center 08:28:37.828 +53:58:46.52
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 08:28:35.074 +53:59:05.08
Second-epoch second image center 08:28:37.828 +53:58:46.52
Angular distance between the image centers 0.00849 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits &> /tmp/tmp.gt43J7DWW1
Parallel run for /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits &> /tmp/tmp.AH6KEZDdI6
Parallel run for /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits &> /tmp/tmp.z3feicjVt9
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits &> /tmp/tmp.D80lzJFpUr
Parallel run for /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Calibrating the magnitude scale
Found non-empty wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits and wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits and wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat
Found non-empty wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits and wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat
The reference image (wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits) and catalog (wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat) found
'wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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 29 out of 62506 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 21.714976
a=0.000000 b=1.000000 c=21.714976
From vast_summary.log: estimated ref. image limiting mag.: -7.18
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.53
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.53
____ End of magnitude calibration ____
Filter-out faint candidates...
Filter-out suspiciously bright candidates...
Filter-out candidates with large difference between measured mags in one epoch...
Filter-out small-amplitude flares...
Preparing the exclusion lists for this field
Done with filtering
Found 121 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.0 pix Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
1.9 pix Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
2.0 pix fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
2.0 pix fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Limiting magnitude estimates:
14.5 mag. Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
14.5 mag. Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
14.5 mag. fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
14.5 mag. fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
All-image limiting magnitude estimate: 14.5 (SNR ) 13.8 (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.gt43J7DWW1 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
verification OK: /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits has a WCS header - will blindly trust it is good...
'/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits' -> 'wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits'
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
WCS-calibrated image found: wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
Checking if the catalog wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
WCS catalog name: wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=23, blended=3425, passed=62483
Got 62483 stars (including 58942 good ones) from the SExtractor catalog wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat
util/solve_plate_with_UCAC5 got 62483 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.4'
Seting catalog search parameters based on the expected field of view 927.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012881 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010304 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 166 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: 10.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 10.53"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 213 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 10.44"
Estimated accuracy of the plate solution: 7.02"
Excluding outliers - 183 stars left (next iteration limit 141)
The image catalog is written to wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits -region wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.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.AH6KEZDdI6 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits 569.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
verification OK: /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits has a WCS header - will blindly trust it is good...
'/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits' -> 'wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits'
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
WCS_IMAGE_NAME=wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
WCS-calibrated image found: wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
Checking if the catalog wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits alredy exist and is non-empty...
Catalog wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat corresponding to the image wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
WCS catalog name: wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=3444, passed=62607
Got 62607 stars (including 59048 good ones) from the SExtractor catalog wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat
util/solve_plate_with_UCAC5 got 62607 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.3'
Seting catalog search parameters based on the expected field of view 927.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012879 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010303 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 169 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: 9.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 9.89"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 213 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.88"
Estimated accuracy of the plate solution: 7.17"
Excluding outliers - 187 stars left (next iteration limit 143)
The image catalog is written to wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits -region wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.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.z3feicjVt9 (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...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=3484, passed=61175
Got 61175 stars (including 57582 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat
util/solve_plate_with_UCAC5 got 61175 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.4'
Seting catalog search parameters based on the expected field of view 927.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012881 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010304 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 174 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: 9.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 9.31"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 221 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.25"
Estimated accuracy of the plate solution: 6.43"
Excluding outliers - 193 stars left (next iteration limit 149)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.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.D80lzJFpUr (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...
/mnt/usb2/NMW-TexasTech/workdir/vast_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/util/wcs_image_calibration.sh /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE before on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
FITSFILE after on_the_fly=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
verification OK: /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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=/mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
The fraction of blended stars is high!
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=22, blended=3523, passed=61268
Got 61268 stars (including 57630 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat
util/solve_plate_with_UCAC5 got 61268 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 927.5'
Seting catalog search parameters based on the expected field of view 927.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012882 (46.4 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010306 (37.1 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 172 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: 9.64"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 9.21"
ITERATION 02 -- talking to VizieR, this might be slow!
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 221 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.19"
Estimated accuracy of the plate solution: 7.54"
Excluding outliers - 191 stars left (next iteration limit 144)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
You may view it with the command:
ds9 /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.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_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.fits
Saving fully-calibrated image wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /mnt/usb2/NMW-TexasTech/workdir/img_2026-01-18_CI_Lyn-02-Q1b1x1_020035_TTUQ1b1x1_15699_d14uZv48/wcs_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.fits
Preparing the HTML report for the field Lyn-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_local.txt__out16990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77042.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77045.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77158.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77285.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77318.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77347.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77411.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77412.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77435.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77438.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77461.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77491.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77523.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77554.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77597.dat to exclusion_list_local.txt
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Considering the candidate 77016_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77016_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 77018_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77018_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77018_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77018_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77018_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77024_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77024_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (8.8") between the two second-epoch detections
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Considering the candidate 77025_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77025_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 77028_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77028_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 77029_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77029_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77029_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77029_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77029_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77031_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77031_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 77037_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77037_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77037_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77037_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77037_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77039_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77039_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77039_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77039_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77039_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77042_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77042_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77042_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77042_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77042_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77045_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77045_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77045_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77045_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77045_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77048_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77048_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77048_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77048_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77048_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77049_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77049_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 77050_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77050_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 77051_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77051_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77051_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77051_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77051_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77052_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77052_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 77055_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77055_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77055_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77055_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77055_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77056_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77056_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77056_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77056_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77056_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77158_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77158_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77158_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77158_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77158_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77215_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77215_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77215_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77215_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77215_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77236_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77236_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77236_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77236_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77236_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77248_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77248_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 77279_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77279_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 77285_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77285_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77285_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77285_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77285_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77304_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77304_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.8") between the two second-epoch detections
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Considering the candidate 77309_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77309_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
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Considering the candidate 77314_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77314_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 77318_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77318_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77318_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77318_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77318_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77324_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77324_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 77331_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77331_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 77339_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77339_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 77340_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77340_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 77345_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77345_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77345_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77345_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77345_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77347_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77347_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77347_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77347_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77347_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77350_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77350_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 77353_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77353_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77353_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77353_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77353_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77364_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77364_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (12.4") between the two second-epoch detections
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Considering the candidate 77369_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77369_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 77372_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77372_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 77373_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77373_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 77374_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77374_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (12.8") between the two second-epoch detections
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Considering the candidate 77375_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77375_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 77376_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77376_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 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 77379_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77379_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.6") between the two second-epoch detections
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Considering the candidate 77385_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77385_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 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 77386_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77386_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 77390_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77390_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 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 77399_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77399_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (8.8") between the two second-epoch detections
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Considering the candidate 77401_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77401_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 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 77402_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77402_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 77407_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77407_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 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 77408_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77408_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 77411_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77411_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77411_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77411_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77411_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77412_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77412_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77412_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77412_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77412_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77414_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77414_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 77426_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77426_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
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Considering the candidate 77427_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77427_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 77429_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77429_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 77431_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77431_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 77433_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77433_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77433_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77433_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77433_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77435_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77435_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77435_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77435_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77435_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77437_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77437_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 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 77438_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77438_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77438_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77438_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77438_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77440_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77440_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 77442_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77442_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 77444_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77444_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 77445_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77445_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 77447_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77447_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (8.8") between the two second-epoch detections
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Considering the candidate 77448_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77448_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 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 77450_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77450_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 77454_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77454_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 77459_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77459_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 77461_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77461_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77461_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77461_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77461_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77465_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77465_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 77466_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77466_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.7") between the two second-epoch detections
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Considering the candidate 77471_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77471_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 77475_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77475_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 77478_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77478_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 77487_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77487_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 77489_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77489_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
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Considering the candidate 77490_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77490_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 77491_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77491_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77491_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77491_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77491_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77492_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77492_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 77496_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77496_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 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 77503_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77503_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77503_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77503_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77503_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77504_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77504_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 77505_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77505_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 77512_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77512_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 77513_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77513_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
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Considering the candidate 77518_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77518_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (12.3") between the two second-epoch detections
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Considering the candidate 77520_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77520_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 77521_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77521_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 77523_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77523_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77523_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77523_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77523_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77526_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77526_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 77528_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77528_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 77530_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77530_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 77533_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77533_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 77539_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77539_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 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 77542_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77542_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 77545_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77545_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (25.8") between the two second-epoch detections
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Considering the candidate 77548_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77548_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 77549_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77549_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 77554_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77554_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77554_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77554_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77554_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77556_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77556_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.5") between the two second-epoch detections
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Considering the candidate 77559_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77559_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 77560_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77560_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 77561_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77561_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 77563_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77563_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 77566_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77566_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77566_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77566_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77566_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77582_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77582_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 77583_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77583_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 77584_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77584_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 77592_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77592_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 77595_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77595_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 77597_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 77597_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/77597_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/77597_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/77597_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
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Considering the candidate 77599_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77599_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 77601_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77601_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (12.9") between the two second-epoch detections
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Considering the candidate 77603_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77603_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (15.5") between the two second-epoch detections
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Considering the candidate 77626_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 77626_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks
Rejecting candidate due to large distance (11.4") between the two second-epoch detections
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Considering the candidate 16990_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Preparing report for the candidate 16990_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.png to transient_report/16990_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_reference.png
The output file transient_report/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits_preview.png already exist
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.png to transient_report/16990_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery1.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-30-34_20.00sec_-15.00C_LIGHT_0318.png to transient_report/16990_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery2.png
Successfully moved fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319.png to transient_report/16990_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319_discovery3.png
Successfully moved Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.png to transient_report/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits_preview.png
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Considering the candidate 54167_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319
The candidate 54167_fd_Lyn-02-Q1b1x1_2026-01-18_01-31-17_20.00sec_-15.00C_LIGHT_0319 did not pass the final checks