This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7354,12.14,0.05,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 20260222.2354 12.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:24:50.22 +50:03:45.5 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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 02 22.2354* 08 36 24.72 +55 13 26.6 12.4 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,2461093.7354,12.37,0.05,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 20260222.2354 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:36:24.72 +55:13:26.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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 02 22.2354* 08 40 57.08 +50 09 49.7 12.4 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,2461093.7354,12.37,0.05,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 20260222.2354 12.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:40:57.08 +50:09:49.7 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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 02 22.2354* 09 11 17.84 +51 23 09.1 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,2461093.7354,13.98,0.05,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 20260222.2354 13.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:11:17.84 +51:23:09.1 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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,2461093.7354,13.70,0.05,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 20260222.2354 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:29:18.71 +51:45:28.0 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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,2461093.7354,13.79,0.05,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 20260222.2354 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:26:02.38 +58:05:16.3 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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,2461093.7354,13.54,0.05,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 20260222.2354 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:08:52.22 +55:00:51.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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 02 22.2354* 08 44 30.63 +50 12 44.7 13.5 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
target,2461093.7354,13.49,0.05,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 20260222.2354 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:44:30.63 +50:12:44.7 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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 02 22.2354* 08 54 41.44 +53 52 25.4 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,2461093.7354,13.42,0.05,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 20260222.2354 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:54:41.44 +53:52:25.4 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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,2461093.7354,12.67,0.05,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 20260222.2354 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:14:36.79 +57:27:30.9 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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 02 22.2354* 09 10 28.63 +52 41 15.3 10.5 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 1022632748266050688,2461093.7354,10.54,0.05,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 1022632748266050688 20260222.2354 10.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:10:28.63 +52:41:15.3 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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,2461093.7354,13.69,0.05,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 20260222.2354 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:51:23.50 +58:52:01.8 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2354 2461093.7354 13.84 09:07:12.78 +52:33:24.8
165.35962 41.61826 galactic UMa Second-epoch detections are separated by 2.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1016680610788661632 | 09:07:15.60 +52:33:10.3 (Gaia DR3) | ROT (local) | (local) | Gaia3var=VARIABLE SpType: G3 (LAMOST DR5)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2354* 09 07 12.78 +52 33 24.8 13.8 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 1016680610788661632,2461093.7354,13.84,0.05,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 1016680610788661632 20260222.2354 13.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:07:12.78 +52:33:24.8 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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,2461093.7354,13.97,0.05,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 20260222.2354 13.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 07:52:54.77 +58:21:37.2 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2354 2461093.7354 13.88 09:04:07.78 +51:46:47.3
166.47686 41.26340 galactic UMa Second-epoch detections are separated by 0.1" and 5.8 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 1016529084342204800 | 09:04:10.93 +51:47:04.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F4 (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 02 22.2354* 09 04 07.78 +51 46 47.3 13.9 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 1016529084342204800,2461093.7354,13.88,0.05,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 1016529084342204800 20260222.2354 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:04:07.78 +51:46:47.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2354 2461093.7354 13.73 08:48:51.31 +52:46:34.8
165.52830 38.82979 galactic UMa Second-epoch detections are separated by 4.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 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 02 22.2354* 08 48 51.31 +52 46 34.8 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 1029295067176349312,2461093.7354,13.73,0.05,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 20260222.2354 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:48:51.31 +52:46:34.8 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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 02 22.2354* 09 12 42.94 +50 10 52.1 13.8 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,2461093.7354,13.80,0.05,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 20260222.2354 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:12:42.94 +50:10:52.1 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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 02 22.2354* 09 22 33.25 +55 08 54.6 13.8 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,2461093.7354,13.79,0.05,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 20260222.2354 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:22:33.25 +55:08:54.6 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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 02 22.2354* 08 51 51.64 +52 52 22.2 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,2461093.7354,14.04,0.05,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 20260222.2354 14.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:51:51.64 +52:52:22.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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 02 22.2354* 09 16 27.55 +55 28 11.3 13.9 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,2461093.7354,13.88,0.05,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 20260222.2354 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:16:27.55 +55:28:11.3 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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 02 22.2354* 08 58 14.16 +48 22 17.3 13.9 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,2461093.7354,13.88,0.05,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 20260222.2354 13.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:58:14.16 +48:22:17.3 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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 02 22.2354* 09 01 02.56 +57 21 11.5 13.9 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,2461093.7354,13.89,0.05,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 20260222.2354 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 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:01:02.56 +57:21:11.5 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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 02 22.2354* 08 59 09.83 +50 00 05.3 13.9 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,2461093.7354,13.95,0.05,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 20260222.2354 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 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:59:09.83 +50:00:05.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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,2461093.7354,13.87,0.05,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 20260222.2354 13.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:26:51.43 +57:40:58.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Lyn-02-Q1b1x1_2025-12-23_04-40-27_20_00sec_-15_00C_LIGHT_0570_fits__*pix.png resample_wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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 02 22.2354* 09 16 53.09 +51 47 09.2 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,2461093.7354,13.99,0.05,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 20260222.2354 13.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 09:16:53.09 +51:47:09.2 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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 02 22.2354* 08 43 04.08 +57 55 56.0 14.1 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,2461093.7354,14.11,0.05,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 20260222.2354 14.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:43:04.08 +57:55:56.0 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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,2461093.7354,14.15,0.05,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 20260222.2354 14.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:27:42.37 +53:25:51.3 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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 02 22.2354* 08 40 56.54 +50 09 56.1 11.6 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,2461093.7354,11.58,0.05,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 20260222.2354 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 08:40:56.54 +50:09:56.1 ;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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_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_2026-02-21_23-39-13_20_00sec_-15_00C_LIGHT_0228_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_2026-02-21_23-38-29_20_00sec_-14_90C_LIGHT_0227_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.94487828 23.12.2025 10:40:27.483 /data_ssd/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 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
Last image: 2461093.73568969 22.02.2026 05:39:13.589 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 10
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: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 11078
Objects passed selection criteria: 11075
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: 10791.5
Average stars matched: 10515.8 (97.4447 %)
Memory usage VmPeak: 116340 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sat Feb 21 23:53:03 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 /data_ssd/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 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
Last image: 2461093.73568969 22.02.2026 05:39:13.589 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 151
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: 33 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 2.0 # minimum number of pixels above threshold
DETECT_THRESH 3.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 3.0 # or , in mag.arcsec-2
SATUR_LEVEL 57000.0 # level (in ADUs) at which arises saturation
GAIN 0.83 # detector gain in e-/ADU
WEIGHT_TYPE BACKGROUND
Total objects detected (at least 2 times): 63373
Objects passed selection criteria: 63175
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: 61381.8
Average stars matched: 59335.8 (96.6668 %)
Memory usage VmPeak: 166228 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 00:06:35 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/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 --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
SExtractor catalog cache: saved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat to cache
SExtractor catalog cache: saved Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.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: 2461093.73517407
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_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
Saving wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits to local_wcs_cache/
'wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits' -> 'local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits'
wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits exists and is non-empty
Saving wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits to local_wcs_cache/
'wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits' -> 'local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.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 08:28:32.342 +53:59:11.91
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 08:28:35.143 +53:58:45.33
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 08:28:32.342 +53:59:11.91
Second-epoch second image center 08:28:35.143 +53:58:45.33
Angular distance between the image centers 0.01008 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits &> /tmp/tmp.iDR2ZY11EN
Parallel run for /data_ssd/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 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits &> /tmp/tmp.NTLKUBrFJf
Parallel run for /data_ssd/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 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.QZzAeKtMsd
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.S66tMV64Ru
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.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 ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 10 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
2.2 pix fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
2.3 pix fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.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_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
15.3 mag. fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.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.iDR2ZY11EN (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/util/wcs_image_calibration.sh /data_ssd/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=/data_ssd/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=/data_ssd/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=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
verification OK: /data_ssd/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 /data_ssd/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...
'/data_ssd/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=/data_ssd/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 /data_ssd/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
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!
UCAC5 search strategy: trying local copy first
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!
UCAC5 search strategy: trying local copy first
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 /data_ssd/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.NTLKUBrFJf (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/util/wcs_image_calibration.sh /data_ssd/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=/data_ssd/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=/data_ssd/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=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
verification OK: /data_ssd/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 /data_ssd/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...
'/data_ssd/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=/data_ssd/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 /data_ssd/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
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!
UCAC5 search strategy: trying local copy first
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!
UCAC5 search strategy: trying local copy first
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 /data_ssd/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.QZzAeKtMsd (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.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_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=803, passed=10813
Got 10813 stars (including 10000 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 10813 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!
UCAC5 search strategy: trying local copy first
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: 9.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 9.84"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 224 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.70"
Estimated accuracy of the plate solution: 6.87"
Excluding outliers - 203 stars left (next iteration limit 154)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.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.S66tMV64Ru (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.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_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=823, passed=10708
Got 10708 stars (including 9876 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 10708 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!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 171 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: 10.23"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 211 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 10.02"
Estimated accuracy of the plate solution: 7.22"
Excluding outliers - 194 stars left (next iteration limit 150)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.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_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits'
Saving fully-calibrated image wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits'
Preparing the HTML report for the field Lyn-02-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out20658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20670.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out20671.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 17s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 3s
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Considering the candidate 20645_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 20645_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
**** FOUND 08:05:37.40 +56:18:40.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20658_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 20658_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 20663_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 20663_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
**** FOUND 09:12:38.47 +56:32:38.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20667_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 20667_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (24.0") between the two second-epoch detections
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Considering the candidate 20668_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 20668_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (18.4") between the two second-epoch detections
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Considering the candidate 20670_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 20670_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20671_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 20671_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20672_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 20672_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 20674_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 20674_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
**** FOUND 08:49:43.94 +54:24:11.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 20675_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 20675_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (10.2") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 20s
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 ####
08:24:50.22 +50:03:45.5
08:36:24.72 +55:13:26.6
08:40:57.08 +50:09:49.7
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
SExtractor catalog cache: saved Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits.cat to cache
SExtractor catalog cache: saved Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.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_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
Creating symlink local_wcs_cache/wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Lyn-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_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits exists and is non-empty
wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.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 08:28:32.342 +53:59:11.91
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 08:28:35.143 +53:58:45.33
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 08:28:32.342 +53:59:11.91
Second-epoch second image center 08:28:35.143 +53:58:45.33
Angular distance between the image centers 0.01008 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits &> /tmp/tmp.phNNNkRkOb
Parallel run for /data_ssd/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 /data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits &> /tmp/tmp.iS6p9l1GP9
Parallel run for /data_ssd/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 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits &> /tmp/tmp.JNZPdtWS23
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits &> /tmp/tmp.evYXy82zvp
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.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 ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 125 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
2.1 pix fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
2.1 pix fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.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_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
14.5 mag. fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.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.phNNNkRkOb (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/util/wcs_image_calibration.sh /data_ssd/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=/data_ssd/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=/data_ssd/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=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-40-27_20.00sec_-15.00C_LIGHT_0570.fits
verification OK: /data_ssd/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 /data_ssd/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...
'/data_ssd/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=/data_ssd/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 /data_ssd/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
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!
UCAC5 search strategy: trying local copy first
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!
UCAC5 search strategy: trying local copy first
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 /data_ssd/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.iS6p9l1GP9 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/util/wcs_image_calibration.sh /data_ssd/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=/data_ssd/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=/data_ssd/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=/data_ssd/NMW-TexasTech/reference_imgs/Lyn-02-Q1b1x1_2025-12-23_04-41-14_20.00sec_-15.00C_LIGHT_0571.fits
verification OK: /data_ssd/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 /data_ssd/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...
'/data_ssd/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=/data_ssd/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 /data_ssd/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
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!
UCAC5 search strategy: trying local copy first
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!
UCAC5 search strategy: trying local copy first
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 /data_ssd/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.JNZPdtWS23 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.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_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=3676, passed=61012
Got 61012 stars (including 57212 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.cat
util/solve_plate_with_UCAC5 got 61012 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!
UCAC5 search strategy: trying local copy first
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: 8.83"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 9.12"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 224 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.10"
Estimated accuracy of the plate solution: 6.71"
Excluding outliers - 202 stars left (next iteration limit 150)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.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.evYXy82zvp (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
WCS_IMAGE_NAME=wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
WCS-calibrated image found: wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
Checking if the catalog wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits alredy exist and is non-empty...
Catalog wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits.cat corresponding to the image wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.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_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
WCS catalog name: wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=44, blended=3697, passed=61090
Got 61090 stars (including 57289 good ones) from the SExtractor catalog wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits.cat
util/solve_plate_with_UCAC5 got 61090 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!
UCAC5 search strategy: trying local copy first
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: 9.68"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 9.99"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 217 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 9.89"
Estimated accuracy of the plate solution: 7.19"
Excluding outliers - 195 stars left (next iteration limit 148)
The image catalog is written to wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits -region wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.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_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-38-29_20.00sec_-14.90C_LIGHT_0227.fits
Saving fully-calibrated image wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Lyn-02-Q1b1x1_234020_TTUQ1b1x1_14337_hR60jM2A/wcs_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228.fits
Preparing the HTML report for the field Lyn-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_local.txt__out50114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77029.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77033.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77052.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77062.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77290.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77323.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77340.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77341.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77343.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77374.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77375.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77387.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77444.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77536.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77549.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 52s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 18s
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Considering the candidate 77014_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77014_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77025_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77025_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 77026_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77026_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77027_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77027_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77028_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77028_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77029_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77029_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77031_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77031_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77032_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77032_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 77033_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77033_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77036_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77036_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77038_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77038_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77043_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77043_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 77044_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77044_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 77048_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77048_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 77052_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77052_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77057_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77057_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77058_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77058_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 77061_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77061_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77062_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77062_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77119_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77119_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77125_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77125_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (24.4") between the two second-epoch detections
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Considering the candidate 77127_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77127_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (18.6") between the two second-epoch detections
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Considering the candidate 77142_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77142_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 77148_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77148_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77169_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77169_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77188_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77188_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (17.4") between the two second-epoch detections
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Considering the candidate 77196_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77196_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77208_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77208_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77211_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77211_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 77222_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77222_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (17.3") between the two second-epoch detections
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Considering the candidate 77229_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77229_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77235_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77235_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (23.5") between the two second-epoch detections
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Considering the candidate 77251_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77251_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 77265_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77265_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 77268_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77268_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77270_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77270_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 77276_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77276_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 77277_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77277_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 77280_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77280_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77282_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77282_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77290_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77290_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77292_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77292_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (16.0") between the two second-epoch detections
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Considering the candidate 77294_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77294_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
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Considering the candidate 77296_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77296_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77302_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77302_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 77304_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77304_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 77312_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77312_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77320_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77320_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (16.6") between the two second-epoch detections
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Considering the candidate 77323_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77323_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77324_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77324_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77325_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77325_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77326_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77326_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 77328_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77328_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77333_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77333_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77335_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77335_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77337_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77337_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 77340_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77340_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77341_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77341_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77343_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77343_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77346_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77346_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 77352_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77352_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 77353_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77353_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 77359_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77359_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77364_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77364_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77365_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77365_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (20.5") between the two second-epoch detections
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Considering the candidate 77371_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77371_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (17.7") between the two second-epoch detections
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Considering the candidate 77373_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77373_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (19.8") between the two second-epoch detections
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Considering the candidate 77374_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77374_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77375_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77375_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77381_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77381_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77382_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77382_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 77387_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77387_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77389_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77389_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 77391_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77391_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 77392_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77392_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 77408_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77408_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77410_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77410_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (20.4") between the two second-epoch detections
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Considering the candidate 77412_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77412_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 77415_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77415_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 77417_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77417_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (22.3") between the two second-epoch detections
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Considering the candidate 77421_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77421_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (19.1") between the two second-epoch detections
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Considering the candidate 77424_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77424_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77430_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77430_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 77434_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77434_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77436_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77436_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 77438_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77438_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (18.8") between the two second-epoch detections
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Considering the candidate 77443_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77443_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 77444_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77444_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
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Considering the candidate 77445_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77445_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (19.4") between the two second-epoch detections
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Considering the candidate 77448_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77448_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 77450_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77450_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 77451_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77451_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
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Considering the candidate 77455_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77455_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 77456_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77456_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 77457_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77457_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (19.2") between the two second-epoch detections
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Considering the candidate 77461_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77461_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77468_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77468_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 77470_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77470_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 77472_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77472_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
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Considering the candidate 77482_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77482_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77488_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77488_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 77491_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77491_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (17.1") between the two second-epoch detections
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Considering the candidate 77493_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77493_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77496_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77496_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 77498_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77498_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 77499_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77499_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77500_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77500_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77503_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77503_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77508_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77508_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (21.5") between the two second-epoch detections
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Considering the candidate 77509_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77509_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77514_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77514_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 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 77515_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77515_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 77516_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77516_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (16.1") between the two second-epoch detections
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Considering the candidate 77521_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77521_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (23.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77522_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77522_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77525_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77525_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77527_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77527_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (15.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77533_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77533_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (18.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77536_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77536_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77541_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77541_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77544_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 77544_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
Rejecting candidate due to large distance (17.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77545_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77545_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77549_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 77549_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 50114_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
Preparing report for the candidate 50114_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16990_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228
The candidate 16990_fd_Lyn-02-Q1b1x1_2026-02-21_23-39-13_20.00sec_-15.00C_LIGHT_0228 did not pass the final checks
**** FOUND 08:05:37.25 +56:18:41.7 in the exclusion list exclusion_list.txt ****
make_report_in_HTML.sh Phase 2 (HTML assembly): 3s
make_report_in_HTML.sh TOTAL: 73s
Prepared the HTML report for the field Lyn-02-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
08:24:50.22 +50:03:45.5
08:36:24.72 +55:13:26.6
08:40:57.08 +50:09:49.7
08:40:56.54 +50:09:56.1
09:11:17.84 +51:23:09.1
08:29:18.71 +51:45:28.0
08:26:02.38 +58:05:16.3
08:08:52.22 +55:00:51.2
08:44:30.63 +50:12:44.7
08:54:41.44 +53:52:25.4
08:14:36.79 +57:27:30.9
09:10:28.63 +52:41:15.3
07:51:23.50 +58:52:01.8
09:07:12.78 +52:33:24.8
07:52:54.77 +58:21:37.2
09:04:07.78 +51:46:47.3
08:48:51.31 +52:46:34.8
09:12:42.94 +50:10:52.1
09:22:33.25 +55:08:54.6
08:51:51.64 +52:52:22.2
09:16:27.55 +55:28:11.3
08:58:14.16 +48:22:17.3
09:01:02.56 +57:21:11.5
08:59:09.83 +50:00:05.3
08:26:51.43 +57:40:58.5
09:16:53.09 +51:47:09.2
08:43:04.08 +57:55:56.0
08:27:42.37 +53:25:51.3
########### Completed Lyn-02-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
08:24:50.22 +50:03:45.5
08:36:24.72 +55:13:26.6
08:40:57.08 +50:09:49.7
09:11:17.84 +51:23:09.1
08:29:18.71 +51:45:28.0
08:26:02.38 +58:05:16.3
08:08:52.22 +55:00:51.2
08:44:30.63 +50:12:44.7
08:54:41.44 +53:52:25.4
08:14:36.79 +57:27:30.9
09:10:28.63 +52:41:15.3
07:51:23.50 +58:52:01.8
09:07:12.78 +52:33:24.8
07:52:54.77 +58:21:37.2
09:04:07.78 +51:46:47.3
08:48:51.31 +52:46:34.8
09:12:42.94 +50:10:52.1
09:22:33.25 +55:08:54.6
08:51:51.64 +52:52:22.2
09:16:27.55 +55:28:11.3
08:58:14.16 +48:22:17.3
09:01:02.56 +57:21:11.5
08:59:09.83 +50:00:05.3
08:26:51.43 +57:40:58.5
09:16:53.09 +51:47:09.2
08:43:04.08 +57:55:56.0
08:27:42.37 +53:25:51.3
08:40:56.54 +50:09:56.1
###################################################################################
08:24:50.22 +50:03:45.5 -- not an asteroid (will add it to exclusion list)
08:36:24.72 +55:13:26.6 -- not an asteroid (will add it to exclusion list)
08:40:57.08 +50:09:49.7 -- not an asteroid (will add it to exclusion list)
09:11:17.84 +51:23:09.1 -- not an asteroid (will add it to exclusion list)
08:29:18.71 +51:45:28.0 -- not an asteroid (will add it to exclusion list)
08:26:02.38 +58:05:16.3 -- not an asteroid (will add it to exclusion list)
08:08:52.22 +55:00:51.2 -- not an asteroid (will add it to exclusion list)
08:44:30.63 +50:12:44.7 -- not an asteroid (will add it to exclusion list)
08:54:41.44 +53:52:25.4 -- not an asteroid (will add it to exclusion list)
08:14:36.79 +57:27:30.9 -- not an asteroid (will add it to exclusion list)
09:10:28.63 +52:41:15.3 -- not an asteroid (will add it to exclusion list)
07:51:23.50 +58:52:01.8 -- not an asteroid (will add it to exclusion list)
09:07:12.78 +52:33:24.8 -- not an asteroid (will add it to exclusion list)
07:52:54.77 +58:21:37.2 -- not an asteroid (will add it to exclusion list)
09:04:07.78 +51:46:47.3 -- not an asteroid (will add it to exclusion list)
08:48:51.31 +52:46:34.8 -- not an asteroid (will add it to exclusion list)
09:12:42.94 +50:10:52.1 -- not an asteroid (will add it to exclusion list)
09:22:33.25 +55:08:54.6 -- not an asteroid (will add it to exclusion list)
08:51:51.64 +52:52:22.2 -- not an asteroid (will add it to exclusion list)
09:16:27.55 +55:28:11.3 -- not an asteroid (will add it to exclusion list)
08:58:14.16 +48:22:17.3 -- not an asteroid (will add it to exclusion list)
09:01:02.56 +57:21:11.5 -- not an asteroid (will add it to exclusion list)
08:59:09.83 +50:00:05.3 -- not an asteroid (will add it to exclusion list)
08:26:51.43 +57:40:58.5 -- not an asteroid (will add it to exclusion list)
09:16:53.09 +51:47:09.2 -- not an asteroid (will add it to exclusion list)
08:43:04.08 +57:55:56.0 -- not an asteroid (will add it to exclusion list)
08:27:42.37 +53:25:51.3 -- not an asteroid (will add it to exclusion list)
08:40:56.54 +50:09:56.1 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
07:51:23.50 +58:52:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
07:52:54.77 +58:21:37.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:08:52.22 +55:00:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:14:36.79 +57:27:30.9 -- does not seem to be a hot pixel (will add it to exclusion list)
08:24:50.22 +50:03:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:26:02.38 +58:05:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:26:51.43 +57:40:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
08:27:42.37 +53:25:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:29:18.71 +51:45:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:36:24.72 +55:13:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
08:40:56.54 +50:09:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
08:40:57.08 +50:09:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:43:04.08 +57:55:56.0 -- does not seem to be a hot pixel (will add it to exclusion list)
08:44:30.63 +50:12:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
08:48:51.31 +52:46:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
08:51:51.64 +52:52:22.2 -- does not seem to be a hot pixel (will add it to exclusion list)
08:54:41.44 +53:52:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
08:58:14.16 +48:22:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
08:59:09.83 +50:00:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:01:02.56 +57:21:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
09:04:07.78 +51:46:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:07:12.78 +52:33:24.8 -- does not seem to be a hot pixel (will add it to exclusion list)
09:10:28.63 +52:41:15.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:11:17.84 +51:23:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:12:42.94 +50:10:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
09:16:27.55 +55:28:11.3 -- does not seem to be a hot pixel (will add it to exclusion list)
09:16:53.09 +51:47:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
09:22:33.25 +55:08:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
07:51:23.50 +58:52:01.8 -- not a known variable star
07:52:54.77 +58:21:37.2 -- not a known variable star
08:08:52.22 +55:00:51.2 -- not a known variable star
08:14:36.79 +57:27:30.9 -- not a known variable star
08:24:50.22 +50:03:45.5 -- not a known variable star
08:26:02.38 +58:05:16.3 -- not a known variable star
08:26:51.43 +57:40:58.5 -- not a known variable star
08:27:42.37 +53:25:51.3 -- not a known variable star
08:29:18.71 +51:45:28.0 -- not a known variable star
08:36:24.72 +55:13:26.6 -- not a known variable star
08:40:56.54 +50:09:56.1 -- not a known variable star
08:40:57.08 +50:09:49.7 -- not a known variable star
08:43:04.08 +57:55:56.0 -- not a known variable star
08:44:30.63 +50:12:44.7 -- not a known variable star
08:48:51.31 +52:46:34.8 -- not a known variable star
08:51:51.64 +52:52:22.2 -- not a known variable star
08:54:41.44 +53:52:25.4 -- not a known variable star
08:58:14.16 +48:22:17.3 -- not a known variable star
08:59:09.83 +50:00:05.3 -- not a known variable star
09:01:02.56 +57:21:11.5 -- not a known variable star
09:04:07.78 +51:46:47.3 -- not a known variable star
09:07:12.78 +52:33:24.8 -- not a known variable star
09:10:28.63 +52:41:15.3 -- a known variable star
09:11:17.84 +51:23:09.1 -- not a known variable star
09:12:42.94 +50:10:52.1 -- not a known variable star
09:16:27.55 +55:28:11.3 -- not a known variable star
09:16:53.09 +51:47:09.2 -- not a known variable star
09:22:33.25 +55:08:54.6 -- not a known variable star
Found 27 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
28 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
###################################################################################
exclusion_list_gaiadr2.txt NOT FOUND
exclusion_list_apass.txt NOT FOUND
IS_THIS_TEST_RUN= NO ALLOW_EXCLUSION_LIST_UPDATE= YES
#### Adding the following to the exclusion list ####
07:51:23.50 +58:52:01.8
07:52:54.77 +58:21:37.2
08:08:52.22 +55:00:51.2
08:14:36.79 +57:27:30.9
08:24:50.22 +50:03:45.5
08:26:02.38 +58:05:16.3
08:26:51.43 +57:40:58.5
08:27:42.37 +53:25:51.3
08:29:18.71 +51:45:28.0
08:36:24.72 +55:13:26.6
08:40:56.54 +50:09:56.1
08:40:57.08 +50:09:49.7
08:43:04.08 +57:55:56.0
08:44:30.63 +50:12:44.7
08:48:51.31 +52:46:34.8
08:51:51.64 +52:52:22.2
08:54:41.44 +53:52:25.4
08:58:14.16 +48:22:17.3
08:59:09.83 +50:00:05.3
09:01:02.56 +57:21:11.5
09:04:07.78 +51:46:47.3
09:07:12.78 +52:33:24.8
09:10:28.63 +52:41:15.3
09:11:17.84 +51:23:09.1
09:12:42.94 +50:10:52.1
09:16:27.55 +55:28:11.3
09:16:53.09 +51:47:09.2
09:22:33.25 +55:08:54.6
####################################################
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461093.73517407 -observatory 500
23:23:34.16 -01:56:53.1 Mercury (-0.1mag)
23:04:46.60 -07:27:50.8 Venus (-3.9mag)
21:43:01.17 -14:51:48.0 Mars (1.1mag)
07:06:05.06 +22:54:21.8 Jupiter (-2.5mag)
00:05:27.88 -01:44:16.6 Saturn (1.0mag)
03:39:59.76 +19:21:44.7 Uranus (5.7mag)
00:03:41.40 -01:01:34.0 Neptune (7.8mag)
20:29:07.54 -22:59:33.0 Pluto (14.5mag)
01:57:52.31 +16:37:55.8 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 362 Feb 21 23:53 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461093.73517407:
07:06:11.09 +22:54:12.1 Io (5.4mag)
07:06:17.56 +22:53:58.3 Europa (5.5mag)
07:05:57.36 +22:54:44.7 Ganymede (4.9mag)
07:06:25.15 +22:53:54.2 Callisto (6.2mag)
07:09:14.34 +23:10:42.8 Himalia (15.0mag)
07:06:08.68 +22:54:16.2 Thebe (15.9mag)
07:08:39.37 +23:19:14.0 Elara (17.0mag)
07:01:38.84 +24:02:17.8 Pasiphae (17.0mag)
07:15:05.94 +22:42:23.1 Carme (18.1mag)
00:05:39.65 -01:44:21.0 Titan (8.8mag)
00:05:33.51 -01:44:15.1 Rhea (10.1mag)
00:05:23.46 -01:45:37.2 Iapetus (11.5mag)
00:05:29.01 -01:44:20.0 Hyperion (14.8mag)
00:07:32.14 -01:31:16.8 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 21 23:53 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461093.73517407:
08:46:24.59 +24:30:47.2 JWST
13:08:50.80 +53:46:17.3 Chandra
16:18:32.20 -53:43:57.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 21 23:53 spacecraft.txt
############################################################
Positions of bright comets (listed at http://astro.vanbuitenen.nl/comets and http://aerith.net/comet/weekly/current.html ) from JPL HORIZONS for JD(UT)2461093.73517407 at 500
16:59:50.98 -11:03:53.0 17.5mag 10P/Tempel 2
03:37:23.42 +28:58:06.2 18.0mag 123P/West-Hartley
08:23:31.16 +60:41:26.1 18.4mag 124P/Mrkos
21:19:50.65 -07:37:26.2 22.1mag 141P/Machholz
01:21:19.68 +11:56:12.9 17.7mag 145P/Shoemaker-Levy 5
11:02:54.41 +30:35:04.8 17.9mag 164P/Christensen
09:33:05.27 -33:51:35.3 18.0mag 195P/Hill
15:52:02.71 -06:35:25.4 19.2mag 210P/Christensen
18:17:13.94 -21:28:13.8 17.3mag 218P/LINEAR
16:21:42.36 -18:10:49.3 15.2mag 235P/LINEAR
03:56:30.28 +27:45:23.9 17.8mag 240P/NEAT
15:17:43.53 +06:38:03.3 14.8mag 24P/Schaumasse
11:23:29.12 -03:23:02.1 17.4mag 29P/Schwassmann-Wachmann 1
07:03:47.26 +27:24:51.6 19.6mag 407P/PanSTARRS-Fuls
17:07:16.78 -11:19:12.0 17.6mag 40P/Vaisala 1
11:02:09.71 -08:51:36.5 16.6mag 43P/Wolf-Harrington
13:25:30.03 -05:49:54.6 20.0mag 489P/Denning
04:34:25.74 +48:34:10.2 17.8mag 493P/2024 Q2 (LONEOS)
06:04:25.10 +47:30:33.6 17.7mag 63P/Wild 1
23:14:46.19 -02:06:37.3 16.2mag 78P/Gehrels 2
20:01:48.49 -22:17:35.5 14.9mag 88P/Howell
15:27:57.09 -29:01:04.1 18.7mag P/2023 S1 (PanSTARRS)
04:43:27.59 -72:35:37.5 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:49.27 +31:12:55.0 18.2mag C/2017 K2 (PanSTARRS)
20:06:40.96 -65:11:47.3 18.1mag C/2020 V2 (ZTF)
17:21:42.47 +04:21:53.7 16.3mag C/2021 G2 (ATLAS)
03:35:44.93 +24:36:48.2 15.8mag C/2022 N2 (PanSTARRS)
09:08:11.56 +29:49:58.3 15.3mag C/2022 QE78 (ATLAS)
08:35:39.07 -06:33:10.7 16.7mag C/2022 R6 (PanSTARRS)
23:53:08.35 +48:26:57.6 18.0mag C/2023 C2 (ATLAS)
09:51:02.40 -20:45:16.2 17.5mag C/2023 F3 (ATLAS)
20:34:55.14 +61:14:31.2 17.3mag C/2023 H5 (Lemmon)
19:34:30.70 -03:24:18.4 16.1mag C/2023 R1 (PANSTARRS)
02:48:56.96 +35:40:31.9 18.5mag C/2023 RS61 (PanSTARRS)
21:01:35.32 +81:20:02.8 18.0mag C/2023 X2 (Lemmon)
06:39:02.58 +63:49:20.2 17.3mag C/2024 A1 (ATLAS)
01:57:21.57 -24:31:02.2 11.2mag C/2024 E1 (Wierzchos)
11:44:54.79 -02:33:54.8 18.1mag C/2024 G2 (ATLAS)
19:28:23.73 +00:39:22.6 19.0mag C/2024 G4 (PanSTARRS)
16:37:11.58 -01:42:14.1 17.7mag C/2024 G6 (ATLAS)
19:53:31.00 +03:16:01.3 15.6mag C/2024 J3 (ATLAS)
02:47:17.23 -31:33:32.6 15.4mag C/2024 T5 (ATLAS)
16:24:52.52 -58:15:43.9 15.6mag C/2025 A6 (Lemmon)
04:50:28.53 +62:12:33.1 16.7mag C/2025 J1 (Borisov)
00:00:00.00 +00:00:00.0 cannot get JPL HORIZONS ephemerides for non-periodic comet C/2025 K1 (ATLAS)
15:56:39.99 -12:57:09.5 14.8mag C/2025 L1 (ATLAS)
02:20:18.31 -19:06:39.9 16.7mag C/2025 Q3 (ATLAS)
02:09:40.84 +17:17:12.4 21.2mag C/2025 R2 (SWAN)
22:20:47.65 +17:39:21.8 16.4mag C/2025 R3 (PANSTARRS)
21:46:06.52 -16:51:28.5 21.5mag C/2025 T1 (ATLAS)
03:06:03.07 -20:31:37.4 18.3mag C/2026 A1 (MAPS)
21:03:20.55 +20:57:52.4 16.9mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.6K Feb 21 23:54 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.72 -74:35:50.10 AT2026ahr 2026-01-20.19 17.09
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:24.99 +04:00:02.20 SN 2026kc 2026-01-18.61 16.1
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
14:46:54.08 -64:04:30.10 ASASSN-26ah 2026-01-15.07 16.84
23:02:43.24 +20:04:53.00 SN2025ajvh 2026-01-15.07 16.03
14:12:27.38 -30:12:29.10 ASASSN-26ag 2026-01-14.27 15.35
14:33:53.58 +05:27:35.40 SN 2025ajnc 2026-01-14.32 15.79
01:43:00.31 -34:11:40.60 AT2025afcm 2026-01-13.08 0.45
00:26:17.71 -52:11:38.60 AT2025ahal 2026-01-11.06 17.57
00:51:36.17 +29:42:40.10 SN2025ahxd 2026-01-11.21 15
10:19:19.14 -37:54:58.30 AT2025ahrt 2026-01-10.26 -0.54
14:37:48.78 +15:51:04.20 SN2025ajng 2026-01-9.42 16.35
05:01:03.70 -08:34:13.20 SN2026A 2026-01-9.28 16.83
00:02:52.11 +13:05:42.90 SN2025ajvg 2026-01-9.13 15.89
08:37:09.62 -02:18:08.80 SN2025aigm 2026-01-9.55 17.66
09:52:50.71 +39:36:55.70 SN2025ahyt 2026-01-9.37 16.97
11:22:19.08 -27:21:40.90 AT2026ta 2026-01-9.32 15.88
14:35:00.21 +00:59:11.40 SN 2025ahsa 2026-01-8.35 -2
09:25:42.42 +22:20:06.10 SN2025ahkt 2026-01-8.03 15.88
22:39:53.44 +34:53:50.00 SN 2025aikz 2026-01-7.09 16.3
08:21:20.95 +20:52:01.60 SN 2025aiks 2026-01-7.13 15.82
07:35:31.38 +09:10:32.40 AT2025ajvk 2026-01-7.12 -1.82
02:50:07.71 -16:37:02.30 AT2026nl 2026-01-7.16 14.19
14:05:12.75 -33:46:00.80 SN 2025ajmj 2026-01-7.31 14.93
12:35:08.33 +28:03:22.70 SN 2025aiaj 2026-01-5.44 15.76
05:30:00.47 -66:43:29.40 ASASSN-26af 2026-01-5.12 14.38
14:05:05.13 -44:14:24.00 ASASSN-26ac 2026-01-5.3 16.01
11:29:16.57 +20:35:09.00 AT2025alco 2026-01-4.39 15.93
16:42:59.28 +26:21:02.80 ASASSN-26ae 2026-01-4.52 14.31
04:13:46.60 -05:02:16.60 ASASSN-26ad 2026-01-4.32 14.58
05:00:01.32 -57:14:29.70 ASASSN-25fj/ASASSN-26ab 2026-01-1.19 13.38
13:53:51.35 -17:55:38.10 ASASSN-25fg 2025-12-23.33 16.66
06:18:15.27 +15:47:38.10 AT2025ahtd 2025-12-23.31 16.96
07:20:53.12 -33:02:58.20 SN 2025agvw 2025-12-23.32 16.84
02:58:15.63 +44:47:45.80 ASASSN-25fh 2025-12-23.13 15.63
04:51:03.78 -36:13:59.00 AT2025aftm 2025-12-20.14 17.35
03:12:59.31 +17:41:45.20 SN2025afzm 2025-12-20.15 17.22
13:33:14.27 -46:03:33.90 ASASSN-25fc 2025-12-19.32 SDSS
07:07:30.84 +24:37:55.60 SN2025agie 2025-12-19.19 16.96
12:31:24.34 -59:07:09.00 ASASSN-25fd 2025-12-19.06 14.94
14:02:20.59 -20:28:28.70 ASASSN-25fe 2025-12-19.34 SDSS
08:08:51.65 -16:39:31.50 ASASSN-25ff 2025-12-19.22 SDSS
00:34:05.69 +05:21:07.50 SN2025afty 2025-12-18.21 16.92
01:35:25.55 -05:40:42.00 AT2025agsf 2025-12-18.12 17.67
06:12:00.84 -46:50:40.70 AT2025aetd 2025-12-15.08 17.32
11:07:12.05 -55:12:59.00 ASASSN-25fa 2025-12-14.25 16.07
02:48:09.78 +37:45:17.90 AT2025afje 2025-12-13.28 17.65
08:17:38.99 +59:57:25.90 SN2025afcy 2025-12-13.43 16.8
22:58:25.70 +26:38:19.80 SN 2025afve 2025-12-12.1 16.63
03:44:52.10 -59:08:22.80 SN 2025aegk 2025-12-12.1 SDSS
04:55:47.45 -18:56:49.70 SN 2025aetg 2025-12-11.36 16.92
23:15:07.77 +13:10:19.80 SN 2025afwb 2025-12-11.2 17.13
02:19:39.33 -45:39:00.60 SN 2025aeqg 2025-12-10.07 16.77
02:03:03.89 +04:14:37.30 SN2025afih 2025-12-8.1 16.49
22:23:03.49 -56:35:57.50 AT2025aeei 2025-12-8.03 16.01
-rw-r--r-- 1 apache apache 6.2K Feb 21 23:53 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:45:58.45 +39:05:10.3 TCP J14455845+3905103 2025-12-30.8196 14.1mag
00:43:23.44 +41:24:35.7 PNV J00432344+4124357 2025-12-11.684 19.7mag
00:41:01.11 +41:59:28.2 PNV J00410111+4159282 2026-01-06.1994 18.7mag
00:42:52.01 +41:14:29.2 PNV J00425201+4114292 2026-01-08.7863 18.37Cmag
02:50:07.72 -16:37:02.3 TCP J02500772-1637023 2026-01-06.6352 14.53Cmag
00:42:58.52 +41:14:44.2 PNV J00425852+4114442 2026-01-13.4991 16.89Cmag
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
-rw-r--r-- 1 apache apache 187K Feb 21 23:53 tocp_transients_list.txt