This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY
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,2461082.7721,12.29,0.05,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 20260211.2721 12.29CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:28:22.35 +66:45:24.6 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 12.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:19:13.84 +71:34:27.4 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:00.75 +68:11:12.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:23:24.12 +72:18:06.3 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.78,0.05,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 20260211.2721 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:13:57.33 +65:01:41.1 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.68,0.05,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 20260211.2721 13.68CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:45:23.36 +74:05:31.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.55,0.05,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 20260211.2721 13.55CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:11:09.00 +66:45:16.7 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.62,0.05,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 20260211.2721 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:02.46 +68:42:26.5 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.26,0.05,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 20260211.2721 13.26CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:58.95 +72:15:49.6 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:21:58.18 +66:47:24.6 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 13.31 06:10:22.43 +71:18:00.3
142.88339 22.39934 galactic Cam Second-epoch detections are separated by 5.3" and 8.3 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 1107771266500436480 | 06:10:19.07 +71:18:38.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1107771266500436480,2461082.7721,13.31,0.05,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 1107771266500436480 20260211.2721 13.31CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:22.43 +71:18:00.3 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.39,0.05,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 20260211.2721 13.39CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:42:15.82 +69:41:59.5 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.31,0.05,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 20260211.2721 13.31CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:48.34 +70:42:31.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.40,0.05,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 20260211.2721 13.40CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:44:47.21 +68:01:36.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.41,0.05,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 20260211.2721 13.41CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:31.71 +69:52:29.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.17,0.05,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 20260211.2721 13.17CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:39.99 +68:56:27.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 549885113881858816,2461082.7721,13.22,0.05,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 549885113881858816 20260211.2721 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:03:54.86 +74:16:16.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.09,0.05,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 20260211.2721 13.09CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:00:02.55 +69:39:46.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.26,0.05,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 20260211.2721 13.26CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:06:41.68 +73:54:03.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.27,0.05,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 20260211.2721 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:28.34 +65:50:00.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:05:46.98 +64:54:18.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.94,0.05,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 20260211.2721 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:47:53.83 +71:31:06.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.80,0.05,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 20260211.2721 12.80CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:18:42.89 +64:28:17.5 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 12.71 06:03:05.64 +69:05:56.4
144.88453 21.06948 galactic Cam Second-epoch detections are separated by 1.9" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1105625088524463104 | 06:03:02.99 +69:05:38.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1105625088524463104,2461082.7721,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1105625088524463104 20260211.2721 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:05.64 +69:05:56.4 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 12.65 04:50:49.70 +67:33:03.8
142.87497 14.52023 galactic Cam Second-epoch detections are separated by 6.3" and 7.8 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 483876723580781952 | 04:50:43.32 +67:33:22.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 483876723580781952,2461082.7721,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 483876723580781952 20260211.2721 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:49.70 +67:33:03.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:59.57 +70:59:07.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:12:16.44 +68:44:04.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.48,0.05,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 20260211.2721 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:43:31.71 +64:09:08.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 12.70 03:47:56.04 +67:53:17.2
138.38897 10.48438 galactic Cam Second-epoch detections are separated by 6.2" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 493284557383018368 | 03:47:56.04 +67:53:17.2 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.488+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 493284557383018368,2461082.7721,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 493284557383018368 20260211.2721 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:56.04 +67:53:17.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.62,0.05,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 20260211.2721 12.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:21:41.67 +70:29:13.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 12.48 04:08:39.70 +71:27:13.4
137.34558 14.34323 galactic Cam Second-epoch detections are separated by 6.4" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 501098472989024000 | 04:08:41.25 +71:26:59.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 501098472989024000,2461082.7721,12.48,0.05,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 501098472989024000 20260211.2721 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:08:39.70 +71:27:13.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:49.53 +72:44:22.1 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.25,0.05,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 20260211.2721 12.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:35.34 +65:59:15.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.05,0.05,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 20260211.2721 12.05CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:41:58.65 +66:44:55.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,11.89,0.05,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 20260211.2721 11.89CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:42.66 +72:25:39.1 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 485981738594069888,2461082.7721,11.79,0.05,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
Gaia DR3 485981738594069888 20260211.2721 11.79CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:49.11 +70:34:50.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,11.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 11.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:46:33.85 +73:16:33.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 10.48 03:42:57.37 +65:15:27.4
139.65101 8.11527 galactic Cam Second-epoch detections are separated by 5.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 488508210157299328 | 03:43:01.37 +65:15:40.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 488508210157299328,2461082.7721,10.48,0.05,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 488508210157299328 20260211.2721 10.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:57.37 +65:15:27.4 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,10.81,0.05,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 20260211.2721 10.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:32:24.37 +65:24:04.3 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,10.84,0.05,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
target 20260211.2721 10.84CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:53:15.02 +66:04:05.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 11.71 04:35:14.65 +72:39:22.4
137.87281 16.66090 galactic Cam Second-epoch detections are separated by 3.1" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J043523.69+723918.6 | 04:35:23.69 +72:39:18.6 (Gaia DR3) | SR (local) | 51.300000000000 (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!
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
ASASSN-V J043523.69+723918.6,2461082.7721,11.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J043523.69+723918.6 20260211.2721 11.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:35:14.65 +72:39:22.4 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 12.12 05:00:10.82 +69:55:05.3
141.40731 16.59897 galactic Cam Second-epoch detections are separated by 7.7" and 7.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J075.0249+69.9172 | 05:00:10.82 +69:55:05.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J075.0249+69.9172,2461082.7721,12.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J075.0249+69.9172 20260211.2721 12.12CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:00:10.82 +69:55:05.3 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.11,0.05,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 20260211.2721 12.11CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:28:30.63 +74:00:18.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.30,0.05,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 20260211.2721 12.30CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:31:25.84 +71:29:26.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.44,0.05,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 20260211.2721 12.44CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:10.02 +66:14:18.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:25:28.11 +70:15:10.5 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:42:42.89 +66:30:46.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 12.56 03:44:48.76 +74:36:03.1
133.83610 15.53004 galactic Cam Second-epoch detections are separated by 7.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 550658100617584384 | 03:44:47.05 +74:35:38.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 550658100617584384,2461082.7721,12.56,0.05,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 550658100617584384 20260211.2721 12.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:44:48.76 +74:36:03.1 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:04.67 +66:30:01.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 12.70 05:22:00.12 +74:37:11.0
138.11068 20.47872 galactic Cam Second-epoch detections are separated by 2.6" and 7.8 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 | TYC 4355-850-1 | 05:22:06.28 +74:36:42.9 (Gaia DR3) | SRS (local) | 26.600000000000 (local) | Gaia3var=NOT_AVAILABLE SpType: M2 1947AnDea...5....1L DO 29093
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TYC 4355-850-1,2461082.7721,12.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TYC 4355-850-1 20260211.2721 12.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:22:00.12 +74:37:11.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 12.79 04:37:27.18 +70:01:51.3
140.08987 15.11921 galactic Cam Second-epoch detections are separated by 7.9" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J069.3942+70.0239 | 04:37:27.18 +70:01:51.3 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J069.3942+70.0239,2461082.7721,12.79,0.05,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
ATO J069.3942+70.0239 20260211.2721 12.79CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:37:27.18 +70:01:51.3 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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 11.2721* 03 34 59.53 +71 38 53.8 12.9 U Cas 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 543153422658023040,2461082.7721,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543153422658023040 20260211.2721 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:34:59.53 +71:38:53.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.78,0.05,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 20260211.2721 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:46:34.74 +71:06:42.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.79,0.05,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 20260211.2721 12.79CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:40.97 +68:48:37.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.95,0.05,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 20260211.2721 12.95CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:39:50.40 +74:51:06.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:14:47.82 +68:30:02.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 12.85 05:22:13.44 +65:58:14.5
146.03021 16.19631 galactic Cam Second-epoch detections are separated by 4.0" and 8.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 480883303176816512 | 05:22:09.68 +65:58:47.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 480883303176816512,2461082.7721,12.85,0.05,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 480883303176816512 20260211.2721 12.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:22:13.44 +65:58:14.5 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 495224336415689728,2461082.7721,13.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 495224336415689728 20260211.2721 13.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:02.06 +71:09:25.4 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:25.48 +65:14:00.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.02,0.05,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 20260211.2721 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:12:37.45 +65:13:39.1 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:54:27.37 +67:00:15.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 500296520993681408,2461082.7721,12.98,0.05,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
Gaia DR3 500296520993681408 20260211.2721 12.98CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:18:38.34 +71:09:35.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:41:24.56 +74:33:25.3 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:22.19 +65:10:32.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:29:15.52 +69:32:30.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.11,0.05,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 20260211.2721 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:59:20.59 +74:14:01.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.21,0.05,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 20260211.2721 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:22:44.78 +70:21:33.5 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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 11.2721* 03 29 11.57 +73 23 37.7 13.3 U Cas 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,2461082.7721,13.30,0.05,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 20260211.2721 13.30CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:29:11.57 +73:23:37.7 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.17,0.05,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 20260211.2721 13.17CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:29.91 +65:59:41.1 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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 11.2721* 03 20 15.93 +70 25 18.0 13.3 U Cas 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,2461082.7721,13.29,0.05,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 20260211.2721 13.29CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:20:15.93 +70:25:18.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:40:36.01 +64:27:57.7 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.11,0.05,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 20260211.2721 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:32:50.00 +66:05:09.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:49.36 +70:12:09.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.21,0.05,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 20260211.2721 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:13.47 +70:20:39.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.14,0.05,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 20260211.2721 13.14CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:25:43.87 +64:44:34.5 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.43,0.05,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 20260211.2721 13.43CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:28:27.35 +64:34:39.7 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 13.15 03:35:57.07 +72:27:17.1
134.69584 13.45497 galactic Cas Second-epoch detections are separated by 4.7" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:35:57.07 +72:27:17.1 (user input) | T | P | (position from user input) J-Ks=0.919+/-0.034 (M)
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 11.2721* 03 35 57.07 +72 27 17.1 13.2 U Cas 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,2461082.7721,13.15,0.05,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 20260211.2721 13.15CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:35:57.07 +72:27:17.1 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:38:16.78 +64:18:56.6 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.36,0.05,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 20260211.2721 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:18:33.11 +75:10:21.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.39,0.05,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 20260211.2721 13.39CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:41:57.03 +66:34:14.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.29,0.05,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 20260211.2721 13.29CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:47:22.82 +69:29:01.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 13.31 03:36:02.63 +71:29:39.9
135.29436 12.69181 galactic Cas Second-epoch detections are separated by 5.8" and 7.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:36:02.63 +71:29:39.9 (user input) | T | P | (position from user input) J-Ks=0.418+/-0.032 (G)
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 11.2721* 03 36 02.63 +71 29 39.9 13.3 U Cas 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,2461082.7721,13.31,0.05,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 20260211.2721 13.31CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:36:02.63 +71:29:39.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.30,0.05,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 20260211.2721 13.30CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:53.60 +71:43:25.7 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.37,0.05,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 20260211.2721 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:39.82 +68:26:59.3 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.30,0.05,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 20260211.2721 13.30CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:15:49.01 +75:03:37.5 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.48,0.05,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 20260211.2721 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:21:31.94 +65:18:29.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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 11.2721* 03 07 32.46 +74 40 41.7 13.4 U Cas 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,2461082.7721,13.37,0.05,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 20260211.2721 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:07:32.46 +74:40:41.7 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.34,0.05,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 20260211.2721 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:08:03.56 +70:03:37.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.43,0.05,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 20260211.2721 13.43CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:16:48.34 +69:53:53.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 489102835490184064,2461082.7721,13.49,0.05,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
Gaia DR3 489102835490184064 20260211.2721 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:06:53.80 +65:28:57.3 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.32,0.05,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 20260211.2721 13.32CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:18:43.49 +70:20:51.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.40,0.05,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 20260211.2721 13.40CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:55:43.67 +74:31:22.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.29,0.05,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 20260211.2721 13.29CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:43:02.04 +70:23:05.6 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.32,0.05,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 20260211.2721 13.32CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:46:22.00 +67:39:08.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.48,0.05,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 20260211.2721 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:34.61 +67:47:21.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:32.67 +73:24:00.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.56,0.05,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 20260211.2721 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:40:16.00 +63:55:28.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 13.43 04:22:24.45 +70:55:21.0
138.53826 14.76383 galactic Cam Second-epoch detections are separated by 8.5" and 7.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 500228901027633792 | 04:22:20.68 +70:55:47.7 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 500228901027633792,2461082.7721,13.43,0.05,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
Large-amplitude variable Gaia DR2 500228901027633792 20260211.2721 13.43CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:22:24.45 +70:55:21.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:55.85 +67:06:40.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 479785372095114880,2461082.7721,13.55,0.05,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 479785372095114880 20260211.2721 13.55CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:32:37.99 +64:30:44.3 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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 11.2721* 03 15 17.05 +71 56 29.2 13.5 U Cas 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,2461082.7721,13.53,0.05,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 20260211.2721 13.53CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:15:17.05 +71:56:29.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 13.56 04:24:09.29 +67:35:46.5
141.15029 12.60792 galactic Cam Second-epoch detections are separated by 7.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:24:09.29 +67:35:46.5 (user input) | T | P | (position from user input) J-Ks=0.795+/-0.165 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461082.7721,13.56,0.05,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 20260211.2721 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:09.29 +67:35:46.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.49,0.05,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 20260211.2721 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:05:06.66 +68:52:52.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.63,0.05,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 20260211.2721 13.63CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:43.54 +70:50:13.7 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.52,0.05,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 20260211.2721 13.52CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:41:42.62 +63:30:22.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 13.52 03:53:09.50 +70:03:44.6
137.33721 12.45520 galactic Cam Second-epoch detections are separated by 6.5" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J058.2880+70.0717 | 03:53:09.50 +70:03:44.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J058.2880+70.0717,2461082.7721,13.52,0.05,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
ATO J058.2880+70.0717 20260211.2721 13.52CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:09.50 +70:03:44.6 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.40,0.05,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 20260211.2721 13.40CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:30:16.59 +67:38:59.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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 11.2721* 03 24 51.02 +69 28 22.4 13.5 U Cas 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,2461082.7721,13.52,0.05,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 20260211.2721 13.52CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:24:51.02 +69:28:22.4 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 13.43 03:36:29.83 +72:18:51.0
134.81683 13.36767 galactic Cas Second-epoch detections are separated by 5.6" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:36:29.83 +72:18:51.0 (user input) | T | P | (position from user input) J-Ks=0.577+/-0.036 (K)
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 11.2721* 03 36 29.83 +72 18 51.0 13.4 U Cas 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,2461082.7721,13.43,0.05,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 20260211.2721 13.43CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:36:29.83 +72:18:51.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.40,0.05,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 20260211.2721 13.40CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:31:43.24 +67:50:04.4 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 13.45 05:15:21.85 +74:29:24.2
138.00062 20.02989 galactic Cam Second-epoch detections are separated by 5.3" and 7.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 502606453187351296 | 05:15:12.93 +74:29:22.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 502606453187351296,2461082.7721,13.45,0.05,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 502606453187351296 20260211.2721 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:21.85 +74:29:24.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.44,0.05,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 20260211.2721 13.44CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:29:51.32 +67:46:46.4 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:36.92 +66:47:24.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.49,0.05,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 20260211.2721 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:36.27 +68:36:55.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.63,0.05,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 20260211.2721 13.63CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:44:04.04 +71:24:17.1 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 13.45 03:44:17.22 +74:14:57.2
134.03854 15.23543 galactic Cam Second-epoch detections are separated by 7.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:44:17.22 +74:14:57.2 (user input) | T | P | (position from user input) J-Ks=0.417+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461082.7721,13.45,0.05,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 20260211.2721 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:44:17.22 +74:14:57.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.61,0.05,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 20260211.2721 13.61CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:18:08.92 +65:16:25.3 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.52,0.05,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 20260211.2721 13.52CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:43.60 +65:00:07.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 13.68 03:44:40.94 +73:01:04.9
134.86404 14.29764 galactic Cam Second-epoch detections are separated by 5.8" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:44:40.94 +73:01:04.9 (user input) | T | P | (position from user input) J-Ks=0.490+/-0.041 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461082.7721,13.68,0.05,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 20260211.2721 13.68CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:44:40.94 +73:01:04.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.45,0.05,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 20260211.2721 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:27:09.03 +68:03:29.6 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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 11.2721* 03 07 11.65 +73 06 25.8 13.6 U Cas 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,2461082.7721,13.56,0.05,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 20260211.2721 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:07:11.65 +73:06:25.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.48,0.05,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 20260211.2721 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:30:25.09 +64:47:15.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 13.48 03:41:55.65 +68:36:20.7
137.49166 10.70037 galactic Cam Second-epoch detections are separated by 7.2" and 6.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:41:55.65 +68:36:20.7 (user input) | T | P | (position from user input) J-Ks=0.442+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461082.7721,13.48,0.05,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 20260211.2721 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:55.65 +68:36:20.7 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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 11.2721* 03 36 50.13 +72 50 02.4 13.5 U Cas 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,2461082.7721,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:36:50.13 +72:50:02.4 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.49,0.05,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 20260211.2721 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:10:47.76 +74:38:43.7 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.61,0.05,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 20260211.2721 13.61CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:16:25.50 +66:23:53.5 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:27.66 +72:21:16.1 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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 11.2721* 03 21 24.13 +70 00 08.5 13.6 U Cas 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,2461082.7721,13.55,0.05,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 20260211.2721 13.55CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:21:24.13 +70:00:08.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:38.21 +67:08:02.7 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.68,0.05,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 20260211.2721 13.68CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:03:17.51 +74:19:32.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:49.87 +69:39:43.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.40,0.05,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 20260211.2721 13.40CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:59:26.53 +73:46:07.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 13.57 05:33:48.21 +66:47:42.0
145.88059 17.61172 galactic Cam Second-epoch detections are separated by 5.5" and 8.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 481025896089879680 | 05:33:45.43 +66:47:10.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 481025896089879680,2461082.7721,13.57,0.05,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 481025896089879680 20260211.2721 13.57CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:33:48.21 +66:47:42.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.39,0.05,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 20260211.2721 13.39CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:56.93 +70:34:39.3 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.57,0.05,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 20260211.2721 13.57CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:14.32 +67:23:36.5 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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 11.2721* 03 21 40.70 +71 10 24.1 13.4 U Cas 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,2461082.7721,13.44,0.05,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 20260211.2721 13.44CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:21:40.70 +71:10:24.1 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.37,0.05,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 20260211.2721 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:49.78 +67:39:43.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.61,0.05,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 20260211.2721 13.61CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:27.42 +72:15:48.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 13.48 05:12:16.81 +65:01:01.6
146.29878 14.81605 galactic Cam Second-epoch detections are separated by 8.8" and 8.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J078.0922+65.0148 | 05:12:16.81 +65:01:01.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ATO J078.0922+65.0148,2461082.7721,13.48,0.05,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
ATO J078.0922+65.0148 20260211.2721 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:12:16.81 +65:01:01.6 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.73,0.05,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
target 20260211.2721 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:22:03.16 +69:45:19.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.52,0.05,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 20260211.2721 13.52CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:34:51.47 +65:20:20.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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 11.2721* 03 07 02.28 +74 32 19.6 13.6 U Cas 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,2461082.7721,13.56,0.05,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 20260211.2721 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:07:02.28 +74:32:19.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.63,0.05,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 20260211.2721 13.63CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:21:14.20 +66:37:09.1 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.52,0.05,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 20260211.2721 13.52CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:33:55.15 +72:58:06.4 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.62,0.05,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 20260211.2721 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:27.03 +66:09:51.7 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.51,0.05,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 20260211.2721 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:47:12.27 +66:16:41.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.57,0.05,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 20260211.2721 13.57CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:51:43.05 +71:34:21.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:12.65 +68:31:49.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 13.68 03:48:25.14 +75:01:30.3
133.74254 16.00715 galactic Cam Second-epoch detections are separated by 5.7" and 7.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:48:25.14 +75:01:30.3 (user input) | T | P | (position from user input) J-Ks=0.452+/-0.048 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461082.7721,13.68,0.05,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 20260211.2721 13.68CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:25.14 +75:01:30.3 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.59,0.05,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 20260211.2721 13.59CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:54.40 +70:02:21.4 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.69,0.05,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 20260211.2721 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:11.95 +72:25:44.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.56,0.05,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 20260211.2721 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:31:56.35 +68:14:17.6 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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 11.2721* 03 31 44.96 +72 28 33.8 13.6 U Cas 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,2461082.7721,13.56,0.05,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 20260211.2721 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:31:44.96 +72:28:33.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:32:01.43 +72:13:09.6 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.62,0.05,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 20260211.2721 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:44:10.25 +72:51:00.7 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:18.52 +65:59:27.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 495103802454134528,2461082.7721,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 495103802454134528 20260211.2721 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:01:42.91 +71:19:23.3 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.73,0.05,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
target 20260211.2721 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:10:28.79 +68:40:36.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.56,0.05,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 20260211.2721 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:57.38 +73:38:58.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544522108477941248,2461082.7721,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544522108477941248 20260211.2721 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:39:59.68 +73:28:51.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.62,0.05,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 20260211.2721 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:06:17.22 +64:56:26.3 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.59,0.05,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 20260211.2721 13.59CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:41:09.80 +66:39:24.1 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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 11.2721* 03 08 20.90 +72 56 20.0 13.7 U Cas 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,2461082.7721,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:20.90 +72:56:20.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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 11.2721* 03 13 12.97 +72 01 17.0 13.7 U Cas 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,2461082.7721,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:13:12.97 +72:01:17.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.77,0.05,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 20260211.2721 13.77CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:50.95 +72:25:41.1 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:19:51.22 +69:21:29.6 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.53,0.05,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 20260211.2721 13.53CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:42.26 +66:43:16.4 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.49,0.05,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 20260211.2721 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:18.39 +68:27:10.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 13.69 04:15:16.04 +73:11:58.4
136.43260 15.93133 galactic Cam Second-epoch detections are separated by 7.7" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 501533261118347136 | 04:15:17.50 +73:11:18.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 501533261118347136,2461082.7721,13.69,0.05,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
Gaia DR3 501533261118347136 20260211.2721 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:15:16.04 +73:11:58.4 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.51,0.05,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 20260211.2721 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:12:59.65 +64:24:34.5 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.56,0.05,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 20260211.2721 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:21.34 +70:17:28.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.57,0.05,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 20260211.2721 13.57CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:53:12.29 +74:45:57.4 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.84,0.05,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
target 20260211.2721 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:09:37.39 +70:37:39.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:45.16 +67:01:17.7 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.68,0.05,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 20260211.2721 13.68CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:57.25 +72:00:29.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.70,0.05,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 20260211.2721 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:09:03.89 +65:59:26.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.58,0.05,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 20260211.2721 13.58CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:16:41.61 +64:43:50.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.62,0.05,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 20260211.2721 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:11:02.06 +71:09:01.8 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:23:33.40 +69:40:42.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.54,0.05,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 20260211.2721 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:20:09.63 +73:47:07.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:44:23.59 +65:05:29.3 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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 11.2721* 03 24 28.84 +69 04 06.1 13.6 U Cas 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,2461082.7721,13.56,0.05,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 20260211.2721 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:24:28.84 +69:04:06.1 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:00:04.08 +71:10:27.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.74,0.05,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 20260211.2721 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:29.07 +68:26:50.6 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.77,0.05,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 20260211.2721 13.77CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:23:17.38 +67:16:34.1 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 13.63 03:55:47.01 +71:26:43.5
136.57588 13.64241 galactic Cam Second-epoch detections are separated by 6.6" and 7.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:55:47.01 +71:26:43.5 (user input) | T | P | (position from user input) J-Ks=0.541+/-0.058 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461082.7721,13.63,0.05,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 20260211.2721 13.63CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:55:47.01 +71:26:43.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.72,0.05,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 20260211.2721 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:57:20.82 +72:06:48.6 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.72,0.05,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 20260211.2721 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:14.96 +67:13:28.6 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.59,0.05,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 20260211.2721 13.59CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:37:08.10 +66:12:52.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 11.2721 2461082.7721 13.77 04:31:03.65 +75:07:21.1
135.69448 18.01849 galactic Cam Second-epoch detections are separated by 3.2" and 6.9 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 550124944854746496 | 04:31:08.95 +75:07:35.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 550124944854746496,2461082.7721,13.77,0.05,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 550124944854746496 20260211.2721 13.77CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:31:03.65 +75:07:21.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260211.2721 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:02:22.38 +74:11:45.5 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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,2461082.7721,13.70,0.05,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 20260211.2721 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:26.62 +72:54:44.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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 11.2721* 03 25 46.70 +69 16 31.2 13.8 U Cas 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,2461082.7721,13.75,0.05,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 20260211.2721 13.75CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:25:46.70 +69:16:31.2 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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 11.2721* 03 30 14.25 +69 49 03.2 13.6 U Cas 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,2461082.7721,13.59,0.05,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 20260211.2721 13.59CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:30:14.25 +69:49:03.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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
IK Cam,2461082.7721,11.54,0.05,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
IK Cam 20260211.2721 11.54CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:03.34 +67:38:47.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0405390+661955,2461082.7721,11.41,0.05,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
NSVS J0405390+661955 20260211.2721 11.41CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:05:39.17 +66:20:03.0 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20_00sec_-15_00C_LIGHT_0258_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20_00sec_-14_90C_LIGHT_0257_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: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
First image: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Last image: 2461082.77232686 11.02.2026 06:31:59.041 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 4
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
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): 16003
Objects passed selection criteria: 15994
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: 15469.2
Average stars matched: 15123.5 (97.7649 %)
Memory usage VmPeak: 120432 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Tue Feb 10 15:05:05 CST 2026
VaST build number 1.0rc88-299-g877bacc0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 00:35:46 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: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
First image: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Last image: 2461082.77232686 11.02.2026 06:31:59.041 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 301
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.31
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: 55 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): 114403
Objects passed selection criteria: 114113
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 109925
Average stars matched: 105846 (96.2893 %)
Memory usage VmPeak: 2071240 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Tue Feb 10 15:05:05 CST 2026
VaST build number 1.0rc88-299-g877bacc0
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-10)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Wed Feb 11 00:46:53 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
SExtractor catalog cache: saved Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat to cache
SExtractor catalog cache: saved Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.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: 2461082.77180627
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits exists and is non-empty
Saving wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits to local_wcs_cache/
'wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> 'local_wcs_cache/wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits'
wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits exists and is non-empty
Saving wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits to local_wcs_cache/
'wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> 'local_wcs_cache/wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits'
wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits'
wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits'
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:47:48.196 +70:00:29.12
Second-epoch image center 04:47:40.089 +70:00:51.04
Angular distance between the image centers 0.01 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 04:47:48.196 +70:00:29.12
Second-epoch image center 04:47:44.272 +70:01:31.49
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 04:47:40.089 +70:00:51.04
Second-epoch second image center 04:47:44.272 +70:01:31.49
Angular distance between the image centers 0.01272 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits &> /tmp/tmp.W7tcZX9Y6s
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits &> /tmp/tmp.P7wXPZykaH
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits &> /tmp/tmp.enpxxdJLlx
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits &> /tmp/tmp.3pfe2RcGZg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Found non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
The reference image (wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits) and catalog (wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat) found
'wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.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 58 out of 16183 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.881698
a=0.000000 b=1.000000 c=22.881698
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.26
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.26
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 4 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
2.1 pix Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
2.1 pix fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
2.1 pix fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
Limiting magnitude estimates:
15.3 mag. Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
15.2 mag. Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
15.2 mag. fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
15.2 mag. fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.W7tcZX9Y6s (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_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> 'wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS-calibrated image found: wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Checking if the catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS catalog name: wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1300, passed=16183
Got 16183 stars (including 14865 good ones) from the SExtractor catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
util/solve_plate_with_UCAC5 got 16183 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.3'
Seting catalog search parameters based on the expected field of view 931.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012935 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010348 (37.3 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 292 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: 6.79"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.09"
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 360 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.02"
Estimated accuracy of the plate solution: 5.56"
Excluding outliers - 323 stars left (next iteration limit 245)
The image catalog is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits -region wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.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.P7wXPZykaH (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_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> 'wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Checking if the catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS catalog name: wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1282, passed=16167
Got 16167 stars (including 14867 good ones) from the SExtractor catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat
util/solve_plate_with_UCAC5 got 16167 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits -region wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.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.enpxxdJLlx (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_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.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_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
Checking if the catalog wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
WCS catalog name: wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1213, passed=14888
Got 14888 stars (including 13653 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits.cat
util/solve_plate_with_UCAC5 got 14888 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.3'
Seting catalog search parameters based on the expected field of view 931.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012935 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010348 (37.3 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 287 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: 6.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.14"
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 344 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.05"
Estimated accuracy of the plate solution: 6.17"
Excluding outliers - 312 stars left (next iteration limit 248)
The image catalog is written to wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits -region wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.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.3pfe2RcGZg (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_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.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_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
Checking if the catalog wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
WCS catalog name: wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1203, passed=14965
Got 14965 stars (including 13748 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits.cat
util/solve_plate_with_UCAC5 got 14965 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.2'
Seting catalog search parameters based on the expected field of view 931.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012933 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010347 (37.2 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 280 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: 6.53"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.02"
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 339 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 5.92"
Estimated accuracy of the plate solution: 6.02"
Excluding outliers - 303 stars left (next iteration limit 237)
The image catalog is written to wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits -region wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.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_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits'
Saving fully-calibrated image wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits'
Preparing the HTML report for the field Cam-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_local.txt__out21021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21070.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 14s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21021_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 21021_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21063_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 21063_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
**** FOUND 03:41:24.35 +72:39:20.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21066_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 21066_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21070_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 21070_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 17s
Prepared the HTML report for the field Cam-06-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 ####
04:28:22.35 +66:45:24.6
05:19:13.84 +71:34:27.4
04:50:00.75 +68:11:12.2
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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
SExtractor catalog cache: saved Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat to cache
SExtractor catalog cache: saved Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Creating symlink local_wcs_cache/wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits exists and is non-empty
wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits exists and is non-empty
wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits exists and is non-empty
wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits exists and is non-empty
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:47:48.196 +70:00:29.12
Second-epoch image center 04:47:40.089 +70:00:51.04
Angular distance between the image centers 0.01 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 04:47:48.196 +70:00:29.12
Second-epoch image center 04:47:44.272 +70:01:31.49
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 04:47:40.089 +70:00:51.04
Second-epoch second image center 04:47:44.272 +70:01:31.49
Angular distance between the image centers 0.01272 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits &> /tmp/tmp.0OOP0vf2b3
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits &> /tmp/tmp.AzOTmFcfYI
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits &> /tmp/tmp.wzOxbl0LBn
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits &> /tmp/tmp.ERlP3WIJi4
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Found non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
The reference image (wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits) and catalog (wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat) found
'wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.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 85 out of 113524 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 21.485425
a=0.000000 b=1.000000 c=21.485425
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.18
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.18
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 259 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
1.9 pix Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
1.9 pix fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
1.9 pix fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
Limiting magnitude estimates:
14.2 mag. Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
14.2 mag. Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
14.1 mag. fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
14.1 mag. fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.4 (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.0OOP0vf2b3 (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_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> 'wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS-calibrated image found: wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Checking if the catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS catalog name: wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=9713, passed=113493
Got 113493 stars (including 103609 good ones) from the SExtractor catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
util/solve_plate_with_UCAC5 got 113493 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.3'
Seting catalog search parameters based on the expected field of view 931.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012935 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010348 (37.3 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 303 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: 6.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.47"
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 368 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.45"
Estimated accuracy of the plate solution: 5.59"
Excluding outliers - 329 stars left (next iteration limit 266)
The image catalog is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits -region wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.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.AzOTmFcfYI (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_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> 'wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Checking if the catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS catalog name: wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=9545, passed=112768
Got 112768 stars (including 103038 good ones) from the SExtractor catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat
util/solve_plate_with_UCAC5 got 112768 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
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 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits -region wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.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.wzOxbl0LBn (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_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.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_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
Checking if the catalog wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
WCS catalog name: wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=45, blended=8959, passed=107799
Got 107799 stars (including 98653 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits.cat
util/solve_plate_with_UCAC5 got 107799 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.3'
Seting catalog search parameters based on the expected field of view 931.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012935 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010348 (37.3 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 296 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: 6.54"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.24"
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 348 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.23"
Estimated accuracy of the plate solution: 5.85"
Excluding outliers - 320 stars left (next iteration limit 260)
The image catalog is written to wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits -region wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.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.ERlP3WIJi4 (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_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.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_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
Checking if the catalog wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
WCS catalog name: wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=33, blended=8926, passed=108200
Got 108200 stars (including 99091 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits.cat
util/solve_plate_with_UCAC5 got 108200 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.2'
Seting catalog search parameters based on the expected field of view 931.2 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012933 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010347 (37.2 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 293 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: 6.04"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 5.99"
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 349 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 5.96"
Estimated accuracy of the plate solution: 5.87"
Excluding outliers - 317 stars left (next iteration limit 256)
The image catalog is written to wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits -region wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.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_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.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_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-14_20.00sec_-14.90C_LIGHT_0257.fits
Saving fully-calibrated image wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.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_2026-02-11_CI_Cam-06-Q1b1x1_003325_TTUQ1b1x1_20041_uKVjOySY/wcs_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258.fits
Preparing the HTML report for the field Cam-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out134061.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134133.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134235.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out133017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133033.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133039.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133057.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133058.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133066.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133071.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133085.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133125.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133249.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133299.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133344.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133351.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133352.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133373.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133391.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133410.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133421.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133431.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133439.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133450.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133465.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133472.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133475.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133484.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133521.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133528.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133537.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133538.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133547.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133560.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133563.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133568.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133572.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133580.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133585.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133588.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133589.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133593.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133605.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133617.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133619.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133621.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133623.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133627.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133633.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133651.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133654.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133659.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133660.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133674.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133685.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133695.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133732.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133743.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133750.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133758.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133759.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133761.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133763.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133785.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133790.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133795.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133800.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133805.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133815.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133817.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133819.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133832.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133834.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133844.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133860.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133865.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133870.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133880.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133883.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133884.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133887.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133896.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133900.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133904.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133909.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133918.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133927.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133945.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133972.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133988.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134002.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134034.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134049.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134092.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134116.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134139.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134147.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134169.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134190.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134191.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134217.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out77457.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90043.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 318s
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: 113s
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Considering the candidate 133016_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133016_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (15.7") between the two second-epoch detections
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Considering the candidate 133017_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133017_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133020_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133020_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133029_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133029_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 133033_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133033_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133039_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133039_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133043_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133043_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133056_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133056_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133057_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133057_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133058_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133058_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133060_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133060_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133061_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133061_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133063_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133063_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 133066_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133066_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133070_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133070_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133071_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133071_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133076_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133076_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (12.7") between the two second-epoch detections
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Considering the candidate 133079_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133079_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133081_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133081_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133084_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133084_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133085_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133085_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133094_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133094_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133104_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133104_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133114_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133114_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133116_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133116_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133118_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133118_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133119_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133119_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133122_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133122_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133123_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133123_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133124_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133124_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133125_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133125_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133126_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133126_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133130_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133130_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133132_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133132_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 133133_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133133_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133135_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133135_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133139_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133139_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133140_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133140_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133141_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133141_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133143_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133143_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133187_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133187_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133190_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133190_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133249_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133249_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133288_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133288_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
**** FOUND 03:41:18.12 +71:26:47.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133299_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133299_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133305_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133305_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133312_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133312_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133344_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133344_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133351_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133351_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133352_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133352_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133373_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133373_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133391_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133391_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133410_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133410_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133419_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133419_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133421_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133421_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133431_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133431_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133439_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133439_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133450_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133450_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133462_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133462_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (12.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133465_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133465_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133467_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133467_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133472_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133472_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133475_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133475_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133484_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133484_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133485_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133485_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133499_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133499_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133508_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133508_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133521_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133521_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133527_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133527_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
**** FOUND 03:36:37.91 +74:56:41.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133528_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133528_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133534_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133534_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
**** FOUND 04:16:54.82 +69:09:52.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133537_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133537_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133538_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133538_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133547_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133547_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133550_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133550_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133558_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133558_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (17.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133560_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133560_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133563_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133563_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133568_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133568_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133572_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133572_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133580_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133580_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133582_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133582_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
**** FOUND 03:43:33.32 +70:59:14.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133585_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133585_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133588_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133588_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133589_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133589_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133593_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133593_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133597_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133597_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133605_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133605_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133606_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133606_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133617_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133617_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133619_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133619_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133621_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133621_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133623_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133623_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133627_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133627_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133633_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133633_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133635_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133635_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133642_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133642_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (11.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133650_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133650_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133651_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133651_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133654_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133654_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133659_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133659_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133660_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133660_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133661_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133661_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
**** FOUND 03:38:54.67 +72:20:29.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133669_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133669_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133674_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133674_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133675_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133675_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133679_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133679_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133681_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133681_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133685_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133685_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133689_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133689_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133690_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133690_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133695_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133695_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133696_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133696_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133702_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133702_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (9.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133705_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133705_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133710_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133710_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133711_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133711_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
**** FOUND 04:02:09.35 +70:45:36.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133721_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133721_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133731_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133731_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133732_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133732_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133743_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133743_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133748_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133748_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (22.7") between the two second-epoch detections
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Considering the candidate 133750_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133750_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133751_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133751_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133757_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133757_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 133758_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133758_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133759_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133759_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133761_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133761_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133763_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133763_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133767_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133767_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 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 133785_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133785_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133790_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133790_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133794_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133794_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133795_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133795_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133800_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133800_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133801_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133801_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133805_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133805_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133806_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133806_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133808_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133808_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133811_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133811_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133815_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133815_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133817_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133817_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133819_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133819_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133827_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133827_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133832_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133832_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133834_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133834_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133836_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133836_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 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 133839_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133839_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 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 133840_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133840_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
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Considering the candidate 133844_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133844_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133845_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133845_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (10.1") between the two second-epoch detections
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Considering the candidate 133850_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133850_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133858_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133858_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133860_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133860_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133862_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133862_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 133863_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133863_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (9.2") between the two second-epoch detections
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Considering the candidate 133865_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133865_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133867_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133867_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 133870_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133870_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133872_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133872_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133877_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133877_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133880_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133880_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133883_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133883_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133884_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133884_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133886_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133886_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 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 133887_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133887_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133894_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133894_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 133896_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133896_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133899_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133899_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133900_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133900_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133902_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133902_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133904_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133904_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133909_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133909_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133910_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133910_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133916_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133916_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (9.3") between the two second-epoch detections
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Considering the candidate 133918_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133918_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133924_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133924_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 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 133927_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133927_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133931_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133931_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133933_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133933_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133934_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133934_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133943_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133943_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133944_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133944_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133945_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133945_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133948_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133948_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 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 133949_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133949_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133951_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133951_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133955_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133955_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133961_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133961_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133968_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133968_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133972_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133972_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133973_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133973_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133975_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133975_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 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 133978_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133978_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133979_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 133979_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 133985_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133985_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133988_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133988_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133990_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133990_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133994_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133994_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133996_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133996_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133997_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 133997_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134001_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134001_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134002_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134002_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134010_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134010_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
**** FOUND 03:53:53.66 +72:16:00.1 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134011_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134011_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134016_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134016_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
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Considering the candidate 134034_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134034_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134036_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134036_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134041_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134041_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
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Considering the candidate 134049_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134049_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134061_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134061_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
**** FOUND 05:38:12.71 +66:17:03.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.79, MAG_FAINT_SEARCH_LIMIT=14.77)GAIADR2_OUTPUT=# 3.882 480554171240573056 084.55036863348 +66.28399861737 14.4217 13.7474 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.882#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134065_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134065_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 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 134067_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134067_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134070_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134070_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134075_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134075_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134082_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134082_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134083_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134083_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134087_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134087_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134089_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134089_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (24.6") between the two second-epoch detections
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Considering the candidate 134092_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134092_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134104_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134104_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134111_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134111_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134115_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134115_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (45.3") between the two second-epoch detections
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Considering the candidate 134116_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134116_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134120_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134120_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 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 134127_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134127_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 134128_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134128_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134129_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134129_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 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 134131_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134131_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 134133_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134133_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
**** FOUND 03:54:28.08 +67:55:39.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.81, MAG_FAINT_SEARCH_LIMIT=14.79)GAIADR2_OUTPUT=# 1.634 493343381259843712 058.61583343908 +67.92764577844 14.7869 13.7570 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.634#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134138_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134138_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134139_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134139_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134141_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134141_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134142_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134142_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134147_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134147_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134148_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134148_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (11.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134151_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134151_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (15.6") between the two second-epoch detections
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Considering the candidate 134153_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134153_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134167_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134167_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134169_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134169_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134172_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134172_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134176_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134176_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
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Considering the candidate 134184_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134184_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
**** FOUND 04:25:21.95 +70:27:48.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134187_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134187_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134190_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134190_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134191_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134191_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134192_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134192_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134201_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134201_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (8.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134206_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134206_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (10.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134211_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134211_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134216_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134216_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134217_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134217_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134228_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134228_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134232_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 134232_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134235_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134235_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
**** FOUND 04:09:06.59 +71:11:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 3.212 501043845303699072 062.28019528505 +71.19082613433 14.5885 13.5791 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.212#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134251_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134251_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134270_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
The candidate 134270_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258 did not pass the final checks
**** FOUND 03:32:14.44 +69:48:52.2 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77457_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 77457_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90043_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
Preparing report for the candidate 90043_fd_Cam-06-Q1b1x1_2026-02-11_00-31-59_20.00sec_-15.00C_LIGHT_0258
make_report_in_HTML.sh Phase 2 (HTML assembly): 23s
make_report_in_HTML.sh TOTAL: 454s
Prepared the HTML report for the field Cam-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:28:22.35 +66:45:24.6
05:19:13.84 +71:34:27.4
04:50:00.75 +68:11:12.2
04:23:24.12 +72:18:06.3
05:13:57.33 +65:01:41.1
04:45:23.36 +74:05:31.9
05:11:09.00 +66:45:16.7
05:03:02.46 +68:42:26.5
06:08:58.95 +72:15:49.6
05:21:58.18 +66:47:24.6
06:10:22.43 +71:18:00.3
05:42:15.82 +69:41:59.5
06:12:48.34 +70:42:31.8
05:44:47.21 +68:01:36.2
06:01:31.71 +69:52:29.2
05:59:39.99 +68:56:27.0
04:03:54.86 +74:16:16.8
05:00:02.55 +69:39:46.9
05:06:41.68 +73:54:03.0
05:58:28.34 +65:50:00.9
05:05:46.98 +64:54:18.9
05:47:53.83 +71:31:06.9
05:18:42.89 +64:28:17.5
06:03:05.64 +69:05:56.4
04:50:49.70 +67:33:03.8
04:56:59.57 +70:59:07.1
05:12:16.44 +68:44:04.1
05:43:31.71 +64:09:08.8
03:47:56.04 +67:53:17.2
04:21:41.67 +70:29:13.2
04:08:39.70 +71:27:13.4
05:34:49.53 +72:44:22.1
05:17:35.34 +65:59:15.0
04:41:58.65 +66:44:55.8
04:24:42.66 +72:25:39.1
05:50:49.11 +70:34:50.0
04:46:33.85 +73:16:33.8
03:42:57.37 +65:15:27.4
05:32:24.37 +65:24:04.3
04:53:15.02 +66:04:05.5
04:35:14.65 +72:39:22.4
05:00:10.82 +69:55:05.3
04:28:30.63 +74:00:18.2
05:31:25.84 +71:29:26.9
05:15:10.02 +66:14:18.2
05:25:28.11 +70:15:10.5
04:42:42.89 +66:30:46.9
03:44:48.76 +74:36:03.1
04:24:04.67 +66:30:01.2
05:22:00.12 +74:37:11.0
04:37:27.18 +70:01:51.3
03:34:59.53 +71:38:53.8
04:46:34.74 +71:06:42.9
05:51:40.97 +68:48:37.8
04:39:50.40 +74:51:06.8
04:14:47.82 +68:30:02.2
05:22:13.44 +65:58:14.5
03:50:02.06 +71:09:25.4
05:54:25.48 +65:14:00.2
05:12:37.45 +65:13:39.1
04:54:27.37 +67:00:15.9
04:18:38.34 +71:09:35.9
04:41:24.56 +74:33:25.3
05:15:22.19 +65:10:32.9
04:29:15.52 +69:32:30.0
04:59:20.59 +74:14:01.2
06:22:44.78 +70:21:33.5
03:29:11.57 +73:23:37.7
05:17:29.91 +65:59:41.1
03:20:15.93 +70:25:18.0
05:40:36.01 +64:27:57.7
05:32:50.00 +66:05:09.2
05:53:49.36 +70:12:09.2
05:34:13.47 +70:20:39.4
05:25:43.87 +64:44:34.5
05:28:27.35 +64:34:39.7
03:35:57.07 +72:27:17.1
05:38:16.78 +64:18:56.6
04:18:33.11 +75:10:21.0
05:41:57.03 +66:34:14.8
04:47:22.82 +69:29:01.0
03:36:02.63 +71:29:39.9
05:49:53.60 +71:43:25.7
05:17:39.82 +68:26:59.3
04:15:49.01 +75:03:37.5
05:21:31.94 +65:18:29.9
03:07:32.46 +74:40:41.7
06:08:03.56 +70:03:37.9
06:16:48.34 +69:53:53.9
04:06:53.80 +65:28:57.3
05:18:43.49 +70:20:51.8
04:55:43.67 +74:31:22.0
05:43:02.04 +70:23:05.6
04:46:22.00 +67:39:08.8
06:05:34.61 +67:47:21.8
03:45:32.67 +73:24:00.0
05:40:16.00 +63:55:28.2
04:22:24.45 +70:55:21.0
05:48:55.85 +67:06:40.2
05:32:37.99 +64:30:44.3
03:15:17.05 +71:56:29.2
04:24:09.29 +67:35:46.5
05:05:06.66 +68:52:52.8
06:07:43.54 +70:50:13.7
05:41:42.62 +63:30:22.8
03:53:09.50 +70:03:44.6
03:30:16.59 +67:38:59.4
03:24:51.02 +69:28:22.4
03:36:29.83 +72:18:51.0
03:31:43.24 +67:50:04.4
05:15:21.85 +74:29:24.2
03:29:51.32 +67:46:46.4
06:02:36.92 +66:47:24.0
05:59:36.27 +68:36:55.9
05:44:04.04 +71:24:17.1
03:44:17.22 +74:14:57.2
05:18:08.92 +65:16:25.3
05:46:43.60 +65:00:07.8
03:44:40.94 +73:01:04.9
03:27:09.03 +68:03:29.6
03:07:11.65 +73:06:25.8
05:30:25.09 +64:47:15.9
03:41:55.65 +68:36:20.7
03:36:50.13 +72:50:02.4
04:10:47.76 +74:38:43.7
05:16:25.50 +66:23:53.5
05:57:27.66 +72:21:16.1
03:21:24.13 +70:00:08.5
05:52:38.21 +67:08:02.7
04:03:17.51 +74:19:32.9
03:54:49.87 +69:39:43.5
03:59:26.53 +73:46:07.8
05:33:48.21 +66:47:42.0
03:42:56.93 +70:34:39.3
03:46:14.32 +67:23:36.5
03:21:40.70 +71:10:24.1
05:52:49.78 +67:39:43.8
06:31:27.42 +72:15:48.2
05:12:16.81 +65:01:01.6
04:22:03.16 +69:45:19.9
04:34:51.47 +65:20:20.5
03:07:02.28 +74:32:19.6
05:21:14.20 +66:37:09.1
04:33:55.15 +72:58:06.4
05:15:27.03 +66:09:51.7
05:47:12.27 +66:16:41.8
04:51:43.05 +71:34:21.8
03:51:12.65 +68:31:49.0
03:48:25.14 +75:01:30.3
05:34:54.40 +70:02:21.4
06:03:11.95 +72:25:44.9
03:31:56.35 +68:14:17.6
03:31:44.96 +72:28:33.8
06:32:01.43 +72:13:09.6
04:44:10.25 +72:51:00.7
04:25:18.52 +65:59:27.9
04:01:42.91 +71:19:23.3
05:10:28.79 +68:40:36.4
05:57:57.38 +73:38:58.0
03:39:59.68 +73:28:51.9
05:06:17.22 +64:56:26.3
05:41:09.80 +66:39:24.1
03:08:20.90 +72:56:20.0
03:13:12.97 +72:01:17.0
06:15:50.95 +72:25:41.1
04:19:51.22 +69:21:29.6
03:56:42.26 +66:43:16.4
05:59:18.39 +68:27:10.2
04:15:16.04 +73:11:58.4
05:12:59.65 +64:24:34.5
05:54:21.34 +70:17:28.9
04:53:12.29 +74:45:57.4
06:09:37.39 +70:37:39.0
05:51:45.16 +67:01:17.7
06:31:57.25 +72:00:29.0
05:09:03.89 +65:59:26.8
05:16:41.61 +64:43:50.8
04:11:02.06 +71:09:01.8
05:23:33.40 +69:40:42.8
05:20:09.63 +73:47:07.1
05:44:23.59 +65:05:29.3
03:24:28.84 +69:04:06.1
04:00:04.08 +71:10:27.0
06:02:29.07 +68:26:50.6
05:23:17.38 +67:16:34.1
03:55:47.01 +71:26:43.5
04:57:20.82 +72:06:48.6
05:07:14.96 +67:13:28.6
05:37:08.10 +66:12:52.0
04:31:03.65 +75:07:21.1
05:02:22.38 +74:11:45.5
05:17:26.62 +72:54:44.0
03:25:46.70 +69:16:31.2
03:30:14.25 +69:49:03.2
03:41:03.34 +67:38:47.0
04:05:39.17 +66:20:03.0
########### Completed Cam-06-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 ####
04:28:22.35 +66:45:24.6
05:19:13.84 +71:34:27.4
04:50:00.75 +68:11:12.2
04:23:24.12 +72:18:06.3
05:13:57.33 +65:01:41.1
04:45:23.36 +74:05:31.9
05:11:09.00 +66:45:16.7
05:03:02.46 +68:42:26.5
06:08:58.95 +72:15:49.6
05:21:58.18 +66:47:24.6
06:10:22.43 +71:18:00.3
05:42:15.82 +69:41:59.5
06:12:48.34 +70:42:31.8
05:44:47.21 +68:01:36.2
06:01:31.71 +69:52:29.2
05:59:39.99 +68:56:27.0
04:03:54.86 +74:16:16.8
05:00:02.55 +69:39:46.9
05:06:41.68 +73:54:03.0
05:58:28.34 +65:50:00.9
05:05:46.98 +64:54:18.9
05:47:53.83 +71:31:06.9
05:18:42.89 +64:28:17.5
06:03:05.64 +69:05:56.4
04:50:49.70 +67:33:03.8
04:56:59.57 +70:59:07.1
05:12:16.44 +68:44:04.1
05:43:31.71 +64:09:08.8
03:47:56.04 +67:53:17.2
04:21:41.67 +70:29:13.2
04:08:39.70 +71:27:13.4
05:34:49.53 +72:44:22.1
05:17:35.34 +65:59:15.0
04:41:58.65 +66:44:55.8
04:24:42.66 +72:25:39.1
05:50:49.11 +70:34:50.0
04:46:33.85 +73:16:33.8
03:42:57.37 +65:15:27.4
05:32:24.37 +65:24:04.3
04:53:15.02 +66:04:05.5
04:35:14.65 +72:39:22.4
05:00:10.82 +69:55:05.3
04:28:30.63 +74:00:18.2
05:31:25.84 +71:29:26.9
05:15:10.02 +66:14:18.2
05:25:28.11 +70:15:10.5
04:42:42.89 +66:30:46.9
03:44:48.76 +74:36:03.1
04:24:04.67 +66:30:01.2
05:22:00.12 +74:37:11.0
04:37:27.18 +70:01:51.3
03:34:59.53 +71:38:53.8
04:46:34.74 +71:06:42.9
05:51:40.97 +68:48:37.8
04:39:50.40 +74:51:06.8
04:14:47.82 +68:30:02.2
05:22:13.44 +65:58:14.5
03:50:02.06 +71:09:25.4
05:54:25.48 +65:14:00.2
05:12:37.45 +65:13:39.1
04:54:27.37 +67:00:15.9
04:18:38.34 +71:09:35.9
04:41:24.56 +74:33:25.3
05:15:22.19 +65:10:32.9
04:29:15.52 +69:32:30.0
04:59:20.59 +74:14:01.2
06:22:44.78 +70:21:33.5
03:29:11.57 +73:23:37.7
05:17:29.91 +65:59:41.1
03:20:15.93 +70:25:18.0
05:40:36.01 +64:27:57.7
05:32:50.00 +66:05:09.2
05:53:49.36 +70:12:09.2
05:34:13.47 +70:20:39.4
05:25:43.87 +64:44:34.5
05:28:27.35 +64:34:39.7
03:35:57.07 +72:27:17.1
05:38:16.78 +64:18:56.6
04:18:33.11 +75:10:21.0
05:41:57.03 +66:34:14.8
04:47:22.82 +69:29:01.0
03:36:02.63 +71:29:39.9
05:49:53.60 +71:43:25.7
05:17:39.82 +68:26:59.3
04:15:49.01 +75:03:37.5
05:21:31.94 +65:18:29.9
03:07:32.46 +74:40:41.7
06:08:03.56 +70:03:37.9
06:16:48.34 +69:53:53.9
04:06:53.80 +65:28:57.3
05:18:43.49 +70:20:51.8
04:55:43.67 +74:31:22.0
05:43:02.04 +70:23:05.6
04:46:22.00 +67:39:08.8
06:05:34.61 +67:47:21.8
03:45:32.67 +73:24:00.0
05:40:16.00 +63:55:28.2
04:22:24.45 +70:55:21.0
05:48:55.85 +67:06:40.2
05:32:37.99 +64:30:44.3
03:15:17.05 +71:56:29.2
04:24:09.29 +67:35:46.5
05:05:06.66 +68:52:52.8
06:07:43.54 +70:50:13.7
05:41:42.62 +63:30:22.8
03:53:09.50 +70:03:44.6
03:30:16.59 +67:38:59.4
03:24:51.02 +69:28:22.4
03:36:29.83 +72:18:51.0
03:31:43.24 +67:50:04.4
05:15:21.85 +74:29:24.2
03:29:51.32 +67:46:46.4
06:02:36.92 +66:47:24.0
05:59:36.27 +68:36:55.9
05:44:04.04 +71:24:17.1
03:44:17.22 +74:14:57.2
05:18:08.92 +65:16:25.3
05:46:43.60 +65:00:07.8
03:44:40.94 +73:01:04.9
03:27:09.03 +68:03:29.6
03:07:11.65 +73:06:25.8
05:30:25.09 +64:47:15.9
03:41:55.65 +68:36:20.7
03:36:50.13 +72:50:02.4
04:10:47.76 +74:38:43.7
05:16:25.50 +66:23:53.5
05:57:27.66 +72:21:16.1
03:21:24.13 +70:00:08.5
05:52:38.21 +67:08:02.7
04:03:17.51 +74:19:32.9
03:54:49.87 +69:39:43.5
03:59:26.53 +73:46:07.8
05:33:48.21 +66:47:42.0
03:42:56.93 +70:34:39.3
03:46:14.32 +67:23:36.5
03:21:40.70 +71:10:24.1
05:52:49.78 +67:39:43.8
06:31:27.42 +72:15:48.2
05:12:16.81 +65:01:01.6
04:22:03.16 +69:45:19.9
04:34:51.47 +65:20:20.5
03:07:02.28 +74:32:19.6
05:21:14.20 +66:37:09.1
04:33:55.15 +72:58:06.4
05:15:27.03 +66:09:51.7
05:47:12.27 +66:16:41.8
04:51:43.05 +71:34:21.8
03:51:12.65 +68:31:49.0
03:48:25.14 +75:01:30.3
05:34:54.40 +70:02:21.4
06:03:11.95 +72:25:44.9
03:31:56.35 +68:14:17.6
03:31:44.96 +72:28:33.8
06:32:01.43 +72:13:09.6
04:44:10.25 +72:51:00.7
04:25:18.52 +65:59:27.9
04:01:42.91 +71:19:23.3
05:10:28.79 +68:40:36.4
05:57:57.38 +73:38:58.0
03:39:59.68 +73:28:51.9
05:06:17.22 +64:56:26.3
05:41:09.80 +66:39:24.1
03:08:20.90 +72:56:20.0
03:13:12.97 +72:01:17.0
06:15:50.95 +72:25:41.1
04:19:51.22 +69:21:29.6
03:56:42.26 +66:43:16.4
05:59:18.39 +68:27:10.2
04:15:16.04 +73:11:58.4
05:12:59.65 +64:24:34.5
05:54:21.34 +70:17:28.9
04:53:12.29 +74:45:57.4
06:09:37.39 +70:37:39.0
05:51:45.16 +67:01:17.7
06:31:57.25 +72:00:29.0
05:09:03.89 +65:59:26.8
05:16:41.61 +64:43:50.8
04:11:02.06 +71:09:01.8
05:23:33.40 +69:40:42.8
05:20:09.63 +73:47:07.1
05:44:23.59 +65:05:29.3
03:24:28.84 +69:04:06.1
04:00:04.08 +71:10:27.0
06:02:29.07 +68:26:50.6
05:23:17.38 +67:16:34.1
03:55:47.01 +71:26:43.5
04:57:20.82 +72:06:48.6
05:07:14.96 +67:13:28.6
05:37:08.10 +66:12:52.0
04:31:03.65 +75:07:21.1
05:02:22.38 +74:11:45.5
05:17:26.62 +72:54:44.0
03:25:46.70 +69:16:31.2
03:30:14.25 +69:49:03.2
03:41:03.34 +67:38:47.0
04:05:39.17 +66:20:03.0
###################################################################################
04:28:22.35 +66:45:24.6 -- not an asteroid (will add it to exclusion list)
05:19:13.84 +71:34:27.4 -- not an asteroid (will add it to exclusion list)
04:50:00.75 +68:11:12.2 -- not an asteroid (will add it to exclusion list)
04:23:24.12 +72:18:06.3 -- not an asteroid (will add it to exclusion list)
05:13:57.33 +65:01:41.1 -- not an asteroid (will add it to exclusion list)
04:45:23.36 +74:05:31.9 -- not an asteroid (will add it to exclusion list)
05:11:09.00 +66:45:16.7 -- not an asteroid (will add it to exclusion list)
05:03:02.46 +68:42:26.5 -- not an asteroid (will add it to exclusion list)
06:08:58.95 +72:15:49.6 -- not an asteroid (will add it to exclusion list)
05:21:58.18 +66:47:24.6 -- not an asteroid (will add it to exclusion list)
06:10:22.43 +71:18:00.3 -- not an asteroid (will add it to exclusion list)
05:42:15.82 +69:41:59.5 -- not an asteroid (will add it to exclusion list)
06:12:48.34 +70:42:31.8 -- not an asteroid (will add it to exclusion list)
05:44:47.21 +68:01:36.2 -- not an asteroid (will add it to exclusion list)
06:01:31.71 +69:52:29.2 -- not an asteroid (will add it to exclusion list)
05:59:39.99 +68:56:27.0 -- not an asteroid (will add it to exclusion list)
04:03:54.86 +74:16:16.8 -- not an asteroid (will add it to exclusion list)
05:00:02.55 +69:39:46.9 -- not an asteroid (will add it to exclusion list)
05:06:41.68 +73:54:03.0 -- not an asteroid (will add it to exclusion list)
05:58:28.34 +65:50:00.9 -- not an asteroid (will add it to exclusion list)
05:05:46.98 +64:54:18.9 -- not an asteroid (will add it to exclusion list)
05:47:53.83 +71:31:06.9 -- not an asteroid (will add it to exclusion list)
05:18:42.89 +64:28:17.5 -- not an asteroid (will add it to exclusion list)
06:03:05.64 +69:05:56.4 -- not an asteroid (will add it to exclusion list)
04:50:49.70 +67:33:03.8 -- not an asteroid (will add it to exclusion list)
04:56:59.57 +70:59:07.1 -- not an asteroid (will add it to exclusion list)
05:12:16.44 +68:44:04.1 -- not an asteroid (will add it to exclusion list)
05:43:31.71 +64:09:08.8 -- not an asteroid (will add it to exclusion list)
03:47:56.04 +67:53:17.2 -- not an asteroid (will add it to exclusion list)
04:21:41.67 +70:29:13.2 -- not an asteroid (will add it to exclusion list)
04:08:39.70 +71:27:13.4 -- not an asteroid (will add it to exclusion list)
05:34:49.53 +72:44:22.1 -- not an asteroid (will add it to exclusion list)
05:17:35.34 +65:59:15.0 -- not an asteroid (will add it to exclusion list)
04:41:58.65 +66:44:55.8 -- not an asteroid (will add it to exclusion list)
04:24:42.66 +72:25:39.1 -- not an asteroid (will add it to exclusion list)
05:50:49.11 +70:34:50.0 -- not an asteroid (will add it to exclusion list)
04:46:33.85 +73:16:33.8 -- not an asteroid (will add it to exclusion list)
03:42:57.37 +65:15:27.4 -- not an asteroid (will add it to exclusion list)
05:32:24.37 +65:24:04.3 -- not an asteroid (will add it to exclusion list)
04:53:15.02 +66:04:05.5 -- not an asteroid (will add it to exclusion list)
04:35:14.65 +72:39:22.4 -- not an asteroid (will add it to exclusion list)
05:00:10.82 +69:55:05.3 -- not an asteroid (will add it to exclusion list)
04:28:30.63 +74:00:18.2 -- not an asteroid (will add it to exclusion list)
05:31:25.84 +71:29:26.9 -- not an asteroid (will add it to exclusion list)
05:15:10.02 +66:14:18.2 -- not an asteroid (will add it to exclusion list)
05:25:28.11 +70:15:10.5 -- not an asteroid (will add it to exclusion list)
04:42:42.89 +66:30:46.9 -- not an asteroid (will add it to exclusion list)
03:44:48.76 +74:36:03.1 -- not an asteroid (will add it to exclusion list)
04:24:04.67 +66:30:01.2 -- not an asteroid (will add it to exclusion list)
05:22:00.12 +74:37:11.0 -- not an asteroid (will add it to exclusion list)
04:37:27.18 +70:01:51.3 -- not an asteroid (will add it to exclusion list)
03:34:59.53 +71:38:53.8 -- not an asteroid (will add it to exclusion list)
04:46:34.74 +71:06:42.9 -- not an asteroid (will add it to exclusion list)
05:51:40.97 +68:48:37.8 -- not an asteroid (will add it to exclusion list)
04:39:50.40 +74:51:06.8 -- not an asteroid (will add it to exclusion list)
04:14:47.82 +68:30:02.2 -- not an asteroid (will add it to exclusion list)
05:22:13.44 +65:58:14.5 -- not an asteroid (will add it to exclusion list)
03:50:02.06 +71:09:25.4 -- not an asteroid (will add it to exclusion list)
05:54:25.48 +65:14:00.2 -- not an asteroid (will add it to exclusion list)
05:12:37.45 +65:13:39.1 -- not an asteroid (will add it to exclusion list)
04:54:27.37 +67:00:15.9 -- not an asteroid (will add it to exclusion list)
04:18:38.34 +71:09:35.9 -- not an asteroid (will add it to exclusion list)
04:41:24.56 +74:33:25.3 -- not an asteroid (will add it to exclusion list)
05:15:22.19 +65:10:32.9 -- not an asteroid (will add it to exclusion list)
04:29:15.52 +69:32:30.0 -- not an asteroid (will add it to exclusion list)
04:59:20.59 +74:14:01.2 -- not an asteroid (will add it to exclusion list)
06:22:44.78 +70:21:33.5 -- not an asteroid (will add it to exclusion list)
03:29:11.57 +73:23:37.7 -- not an asteroid (will add it to exclusion list)
05:17:29.91 +65:59:41.1 -- not an asteroid (will add it to exclusion list)
03:20:15.93 +70:25:18.0 -- not an asteroid (will add it to exclusion list)
05:40:36.01 +64:27:57.7 -- not an asteroid (will add it to exclusion list)
05:32:50.00 +66:05:09.2 -- not an asteroid (will add it to exclusion list)
05:53:49.36 +70:12:09.2 -- not an asteroid (will add it to exclusion list)
05:34:13.47 +70:20:39.4 -- not an asteroid (will add it to exclusion list)
05:25:43.87 +64:44:34.5 -- not an asteroid (will add it to exclusion list)
05:28:27.35 +64:34:39.7 -- not an asteroid (will add it to exclusion list)
03:35:57.07 +72:27:17.1 -- not an asteroid (will add it to exclusion list)
05:38:16.78 +64:18:56.6 -- not an asteroid (will add it to exclusion list)
04:18:33.11 +75:10:21.0 -- not an asteroid (will add it to exclusion list)
05:41:57.03 +66:34:14.8 -- not an asteroid (will add it to exclusion list)
04:47:22.82 +69:29:01.0 -- not an asteroid (will add it to exclusion list)
03:36:02.63 +71:29:39.9 -- not an asteroid (will add it to exclusion list)
05:49:53.60 +71:43:25.7 -- not an asteroid (will add it to exclusion list)
05:17:39.82 +68:26:59.3 -- not an asteroid (will add it to exclusion list)
04:15:49.01 +75:03:37.5 -- not an asteroid (will add it to exclusion list)
05:21:31.94 +65:18:29.9 -- not an asteroid (will add it to exclusion list)
03:07:32.46 +74:40:41.7 -- not an asteroid (will add it to exclusion list)
06:08:03.56 +70:03:37.9 -- not an asteroid (will add it to exclusion list)
06:16:48.34 +69:53:53.9 -- not an asteroid (will add it to exclusion list)
04:06:53.80 +65:28:57.3 -- not an asteroid (will add it to exclusion list)
05:18:43.49 +70:20:51.8 -- not an asteroid (will add it to exclusion list)
04:55:43.67 +74:31:22.0 -- not an asteroid (will add it to exclusion list)
05:43:02.04 +70:23:05.6 -- not an asteroid (will add it to exclusion list)
04:46:22.00 +67:39:08.8 -- not an asteroid (will add it to exclusion list)
06:05:34.61 +67:47:21.8 -- not an asteroid (will add it to exclusion list)
03:45:32.67 +73:24:00.0 -- not an asteroid (will add it to exclusion list)
05:40:16.00 +63:55:28.2 -- not an asteroid (will add it to exclusion list)
04:22:24.45 +70:55:21.0 -- not an asteroid (will add it to exclusion list)
05:48:55.85 +67:06:40.2 -- not an asteroid (will add it to exclusion list)
05:32:37.99 +64:30:44.3 -- not an asteroid (will add it to exclusion list)
03:15:17.05 +71:56:29.2 -- not an asteroid (will add it to exclusion list)
04:24:09.29 +67:35:46.5 -- not an asteroid (will add it to exclusion list)
05:05:06.66 +68:52:52.8 -- not an asteroid (will add it to exclusion list)
06:07:43.54 +70:50:13.7 -- not an asteroid (will add it to exclusion list)
05:41:42.62 +63:30:22.8 -- not an asteroid (will add it to exclusion list)
03:53:09.50 +70:03:44.6 -- not an asteroid (will add it to exclusion list)
03:30:16.59 +67:38:59.4 -- not an asteroid (will add it to exclusion list)
03:24:51.02 +69:28:22.4 -- not an asteroid (will add it to exclusion list)
03:36:29.83 +72:18:51.0 -- not an asteroid (will add it to exclusion list)
03:31:43.24 +67:50:04.4 -- not an asteroid (will add it to exclusion list)
05:15:21.85 +74:29:24.2 -- not an asteroid (will add it to exclusion list)
03:29:51.32 +67:46:46.4 -- not an asteroid (will add it to exclusion list)
06:02:36.92 +66:47:24.0 -- not an asteroid (will add it to exclusion list)
05:59:36.27 +68:36:55.9 -- not an asteroid (will add it to exclusion list)
05:44:04.04 +71:24:17.1 -- not an asteroid (will add it to exclusion list)
03:44:17.22 +74:14:57.2 -- not an asteroid (will add it to exclusion list)
05:18:08.92 +65:16:25.3 -- not an asteroid (will add it to exclusion list)
05:46:43.60 +65:00:07.8 -- not an asteroid (will add it to exclusion list)
03:44:40.94 +73:01:04.9 -- not an asteroid (will add it to exclusion list)
03:27:09.03 +68:03:29.6 -- not an asteroid (will add it to exclusion list)
03:07:11.65 +73:06:25.8 -- not an asteroid (will add it to exclusion list)
05:30:25.09 +64:47:15.9 -- not an asteroid (will add it to exclusion list)
03:41:55.65 +68:36:20.7 -- not an asteroid (will add it to exclusion list)
03:36:50.13 +72:50:02.4 -- not an asteroid (will add it to exclusion list)
04:10:47.76 +74:38:43.7 -- not an asteroid (will add it to exclusion list)
05:16:25.50 +66:23:53.5 -- not an asteroid (will add it to exclusion list)
05:57:27.66 +72:21:16.1 -- not an asteroid (will add it to exclusion list)
03:21:24.13 +70:00:08.5 -- not an asteroid (will add it to exclusion list)
05:52:38.21 +67:08:02.7 -- not an asteroid (will add it to exclusion list)
04:03:17.51 +74:19:32.9 -- not an asteroid (will add it to exclusion list)
03:54:49.87 +69:39:43.5 -- not an asteroid (will add it to exclusion list)
03:59:26.53 +73:46:07.8 -- not an asteroid (will add it to exclusion list)
05:33:48.21 +66:47:42.0 -- not an asteroid (will add it to exclusion list)
03:42:56.93 +70:34:39.3 -- not an asteroid (will add it to exclusion list)
03:46:14.32 +67:23:36.5 -- not an asteroid (will add it to exclusion list)
03:21:40.70 +71:10:24.1 -- not an asteroid (will add it to exclusion list)
05:52:49.78 +67:39:43.8 -- not an asteroid (will add it to exclusion list)
06:31:27.42 +72:15:48.2 -- not an asteroid (will add it to exclusion list)
05:12:16.81 +65:01:01.6 -- not an asteroid (will add it to exclusion list)
04:22:03.16 +69:45:19.9 -- not an asteroid (will add it to exclusion list)
04:34:51.47 +65:20:20.5 -- not an asteroid (will add it to exclusion list)
03:07:02.28 +74:32:19.6 -- not an asteroid (will add it to exclusion list)
05:21:14.20 +66:37:09.1 -- not an asteroid (will add it to exclusion list)
04:33:55.15 +72:58:06.4 -- not an asteroid (will add it to exclusion list)
05:15:27.03 +66:09:51.7 -- not an asteroid (will add it to exclusion list)
05:47:12.27 +66:16:41.8 -- not an asteroid (will add it to exclusion list)
04:51:43.05 +71:34:21.8 -- not an asteroid (will add it to exclusion list)
03:51:12.65 +68:31:49.0 -- not an asteroid (will add it to exclusion list)
03:48:25.14 +75:01:30.3 -- not an asteroid (will add it to exclusion list)
05:34:54.40 +70:02:21.4 -- not an asteroid (will add it to exclusion list)
06:03:11.95 +72:25:44.9 -- not an asteroid (will add it to exclusion list)
03:31:56.35 +68:14:17.6 -- not an asteroid (will add it to exclusion list)
03:31:44.96 +72:28:33.8 -- not an asteroid (will add it to exclusion list)
06:32:01.43 +72:13:09.6 -- not an asteroid (will add it to exclusion list)
04:44:10.25 +72:51:00.7 -- not an asteroid (will add it to exclusion list)
04:25:18.52 +65:59:27.9 -- not an asteroid (will add it to exclusion list)
04:01:42.91 +71:19:23.3 -- not an asteroid (will add it to exclusion list)
05:10:28.79 +68:40:36.4 -- not an asteroid (will add it to exclusion list)
05:57:57.38 +73:38:58.0 -- not an asteroid (will add it to exclusion list)
03:39:59.68 +73:28:51.9 -- not an asteroid (will add it to exclusion list)
05:06:17.22 +64:56:26.3 -- not an asteroid (will add it to exclusion list)
05:41:09.80 +66:39:24.1 -- not an asteroid (will add it to exclusion list)
03:08:20.90 +72:56:20.0 -- not an asteroid (will add it to exclusion list)
03:13:12.97 +72:01:17.0 -- not an asteroid (will add it to exclusion list)
06:15:50.95 +72:25:41.1 -- not an asteroid (will add it to exclusion list)
04:19:51.22 +69:21:29.6 -- not an asteroid (will add it to exclusion list)
03:56:42.26 +66:43:16.4 -- not an asteroid (will add it to exclusion list)
05:59:18.39 +68:27:10.2 -- not an asteroid (will add it to exclusion list)
04:15:16.04 +73:11:58.4 -- not an asteroid (will add it to exclusion list)
05:12:59.65 +64:24:34.5 -- not an asteroid (will add it to exclusion list)
05:54:21.34 +70:17:28.9 -- not an asteroid (will add it to exclusion list)
04:53:12.29 +74:45:57.4 -- not an asteroid (will add it to exclusion list)
06:09:37.39 +70:37:39.0 -- not an asteroid (will add it to exclusion list)
05:51:45.16 +67:01:17.7 -- not an asteroid (will add it to exclusion list)
06:31:57.25 +72:00:29.0 -- not an asteroid (will add it to exclusion list)
05:09:03.89 +65:59:26.8 -- not an asteroid (will add it to exclusion list)
05:16:41.61 +64:43:50.8 -- not an asteroid (will add it to exclusion list)
04:11:02.06 +71:09:01.8 -- not an asteroid (will add it to exclusion list)
05:23:33.40 +69:40:42.8 -- not an asteroid (will add it to exclusion list)
05:20:09.63 +73:47:07.1 -- not an asteroid (will add it to exclusion list)
05:44:23.59 +65:05:29.3 -- not an asteroid (will add it to exclusion list)
03:24:28.84 +69:04:06.1 -- not an asteroid (will add it to exclusion list)
04:00:04.08 +71:10:27.0 -- not an asteroid (will add it to exclusion list)
06:02:29.07 +68:26:50.6 -- not an asteroid (will add it to exclusion list)
05:23:17.38 +67:16:34.1 -- not an asteroid (will add it to exclusion list)
03:55:47.01 +71:26:43.5 -- not an asteroid (will add it to exclusion list)
04:57:20.82 +72:06:48.6 -- not an asteroid (will add it to exclusion list)
05:07:14.96 +67:13:28.6 -- not an asteroid (will add it to exclusion list)
05:37:08.10 +66:12:52.0 -- not an asteroid (will add it to exclusion list)
04:31:03.65 +75:07:21.1 -- not an asteroid (will add it to exclusion list)
05:02:22.38 +74:11:45.5 -- not an asteroid (will add it to exclusion list)
05:17:26.62 +72:54:44.0 -- not an asteroid (will add it to exclusion list)
03:25:46.70 +69:16:31.2 -- not an asteroid (will add it to exclusion list)
03:30:14.25 +69:49:03.2 -- not an asteroid (will add it to exclusion list)
03:41:03.34 +67:38:47.0 -- not an asteroid (will add it to exclusion list)
04:05:39.17 +66:20:03.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
03:07:02.28 +74:32:19.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:07:11.65 +73:06:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:07:32.46 +74:40:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:08:20.90 +72:56:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:13:12.97 +72:01:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:15:17.05 +71:56:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:20:15.93 +70:25:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:21:24.13 +70:00:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:21:40.70 +71:10:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:24:28.84 +69:04:06.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:24:51.02 +69:28:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:25:46.70 +69:16:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:27:09.03 +68:03:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:29:11.57 +73:23:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:29:51.32 +67:46:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:30:14.25 +69:49:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:30:16.59 +67:38:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:31:43.24 +67:50:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:31:44.96 +72:28:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:31:56.35 +68:14:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:59.53 +71:38:53.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:57.07 +72:27:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:02.63 +71:29:39.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:29.83 +72:18:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:50.13 +72:50:02.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:39:59.68 +73:28:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:03.34 +67:38:47.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:55.65 +68:36:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:56.93 +70:34:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:57.37 +65:15:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:17.22 +74:14:57.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:40.94 +73:01:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:48.76 +74:36:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:32.67 +73:24:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:14.32 +67:23:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:56.04 +67:53:17.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:25.14 +75:01:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:02.06 +71:09:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:12.65 +68:31:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:09.50 +70:03:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:49.87 +69:39:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:55:47.01 +71:26:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:56:42.26 +66:43:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:59:26.53 +73:46:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:00:04.08 +71:10:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:01:42.91 +71:19:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:03:17.51 +74:19:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:03:54.86 +74:16:16.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:39.17 +66:20:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:06:53.80 +65:28:57.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:08:39.70 +71:27:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:10:47.76 +74:38:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:11:02.06 +71:09:01.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:14:47.82 +68:30:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:15:16.04 +73:11:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:15:49.01 +75:03:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:18:33.11 +75:10:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:18:38.34 +71:09:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:19:51.22 +69:21:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:21:41.67 +70:29:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:22:03.16 +69:45:19.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:22:24.45 +70:55:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:23:24.12 +72:18:06.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:04.67 +66:30:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:09.29 +67:35:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:42.66 +72:25:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:18.52 +65:59:27.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:28:22.35 +66:45:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:28:30.63 +74:00:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:29:15.52 +69:32:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:31:03.65 +75:07:21.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:55.15 +72:58:06.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:34:51.47 +65:20:20.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:14.65 +72:39:22.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:27.18 +70:01:51.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:39:50.40 +74:51:06.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:41:24.56 +74:33:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:41:58.65 +66:44:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:42:42.89 +66:30:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:44:10.25 +72:51:00.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:45:23.36 +74:05:31.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:46:22.00 +67:39:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:46:33.85 +73:16:33.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:46:34.74 +71:06:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:47:22.82 +69:29:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:50:00.75 +68:11:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:50:49.70 +67:33:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:51:43.05 +71:34:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:12.29 +74:45:57.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:15.02 +66:04:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:27.37 +67:00:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:43.67 +74:31:22.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:59.57 +70:59:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:20.82 +72:06:48.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:20.59 +74:14:01.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:02.55 +69:39:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:10.82 +69:55:05.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:22.38 +74:11:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:02.46 +68:42:26.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:06.66 +68:52:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:46.98 +64:54:18.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:17.22 +64:56:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:41.68 +73:54:03.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:14.96 +67:13:28.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:09:03.89 +65:59:26.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:10:28.79 +68:40:36.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:11:09.00 +66:45:16.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:12:16.44 +68:44:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:12:16.81 +65:01:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:12:37.45 +65:13:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:12:59.65 +64:24:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:13:57.33 +65:01:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:10.02 +66:14:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:21.85 +74:29:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:22.19 +65:10:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:27.03 +66:09:51.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:25.50 +66:23:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:41.61 +64:43:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:26.62 +72:54:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:29.91 +65:59:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:35.34 +65:59:15.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:39.82 +68:26:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:08.92 +65:16:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:42.89 +64:28:17.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:43.49 +70:20:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:13.84 +71:34:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:09.63 +73:47:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:14.20 +66:37:09.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:31.94 +65:18:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:58.18 +66:47:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:00.12 +74:37:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:13.44 +65:58:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:17.38 +67:16:34.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:33.40 +69:40:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:28.11 +70:15:10.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:43.87 +64:44:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:27.35 +64:34:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:25.09 +64:47:15.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:25.84 +71:29:26.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:24.37 +65:24:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:37.99 +64:30:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:50.00 +66:05:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:48.21 +66:47:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:13.47 +70:20:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:49.53 +72:44:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:54.40 +70:02:21.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:08.10 +66:12:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:16.78 +64:18:56.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:16.00 +63:55:28.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:40:36.01 +64:27:57.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:09.80 +66:39:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:42.62 +63:30:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:57.03 +66:34:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:15.82 +69:41:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:02.04 +70:23:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:31.71 +64:09:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:04.04 +71:24:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:23.59 +65:05:29.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:47.21 +68:01:36.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:43.60 +65:00:07.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:12.27 +66:16:41.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:53.83 +71:31:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:55.85 +67:06:40.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:53.60 +71:43:25.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:49.11 +70:34:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:40.97 +68:48:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:45.16 +67:01:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:38.21 +67:08:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:49.78 +67:39:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:49.36 +70:12:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:21.34 +70:17:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:25.48 +65:14:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:27.66 +72:21:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:57.38 +73:38:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:28.34 +65:50:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:18.39 +68:27:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:36.27 +68:36:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:39.99 +68:56:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:31.71 +69:52:29.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:29.07 +68:26:50.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:36.92 +66:47:24.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:05.64 +69:05:56.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:11.95 +72:25:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:34.61 +67:47:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:43.54 +70:50:13.7 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:03.56 +70:03:37.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:08:58.95 +72:15:49.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:37.39 +70:37:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:22.43 +71:18:00.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:48.34 +70:42:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:50.95 +72:25:41.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:16:48.34 +69:53:53.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:44.78 +70:21:33.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:27.42 +72:15:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:57.25 +72:00:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:32:01.43 +72:13:09.6 -- 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)
03:07:02.28 +74:32:19.6 -- not a known variable star
03:07:11.65 +73:06:25.8 -- not a known variable star
03:07:32.46 +74:40:41.7 -- not a known variable star
03:08:20.90 +72:56:20.0 -- not a known variable star
03:13:12.97 +72:01:17.0 -- not a known variable star
03:15:17.05 +71:56:29.2 -- not a known variable star
03:20:15.93 +70:25:18.0 -- not a known variable star
03:21:24.13 +70:00:08.5 -- not a known variable star
03:21:40.70 +71:10:24.1 -- not a known variable star
03:24:28.84 +69:04:06.1 -- not a known variable star
03:24:51.02 +69:28:22.4 -- not a known variable star
03:25:46.70 +69:16:31.2 -- not a known variable star
03:27:09.03 +68:03:29.6 -- not a known variable star
03:29:11.57 +73:23:37.7 -- not a known variable star
03:29:51.32 +67:46:46.4 -- not a known variable star
03:30:14.25 +69:49:03.2 -- not a known variable star
03:30:16.59 +67:38:59.4 -- not a known variable star
03:31:43.24 +67:50:04.4 -- not a known variable star
03:31:44.96 +72:28:33.8 -- not a known variable star
03:31:56.35 +68:14:17.6 -- not a known variable star
03:34:59.53 +71:38:53.8 -- a known variable star
03:35:57.07 +72:27:17.1 -- not a known variable star
03:36:02.63 +71:29:39.9 -- not a known variable star
03:36:29.83 +72:18:51.0 -- not a known variable star
03:36:50.13 +72:50:02.4 -- not a known variable star
03:39:59.68 +73:28:51.9 -- a known variable star
03:41:03.34 +67:38:47.0 -- a known variable star
03:41:55.65 +68:36:20.7 -- not a known variable star
03:42:56.93 +70:34:39.3 -- not a known variable star
03:42:57.37 +65:15:27.4 -- not a known variable star
03:44:17.22 +74:14:57.2 -- not a known variable star
03:44:40.94 +73:01:04.9 -- not a known variable star
03:44:48.76 +74:36:03.1 -- not a known variable star
03:45:32.67 +73:24:00.0 -- not a known variable star
03:46:14.32 +67:23:36.5 -- not a known variable star
03:47:56.04 +67:53:17.2 -- not a known variable star
03:48:25.14 +75:01:30.3 -- not a known variable star
03:50:02.06 +71:09:25.4 -- a known variable star
03:51:12.65 +68:31:49.0 -- not a known variable star
03:53:09.50 +70:03:44.6 -- not a known variable star
03:54:49.87 +69:39:43.5 -- not a known variable star
03:55:47.01 +71:26:43.5 -- not a known variable star
03:56:42.26 +66:43:16.4 -- not a known variable star
03:59:26.53 +73:46:07.8 -- not a known variable star
04:00:04.08 +71:10:27.0 -- not a known variable star
04:01:42.91 +71:19:23.3 -- a known variable star
04:03:17.51 +74:19:32.9 -- not a known variable star
04:03:54.86 +74:16:16.8 -- a known variable star
04:05:39.17 +66:20:03.0 -- a known variable star
04:06:53.80 +65:28:57.3 -- a known variable star
04:08:39.70 +71:27:13.4 -- not a known variable star
04:10:47.76 +74:38:43.7 -- not a known variable star
04:11:02.06 +71:09:01.8 -- not a known variable star
04:14:47.82 +68:30:02.2 -- not a known variable star
04:15:16.04 +73:11:58.4 -- not a known variable star
04:15:49.01 +75:03:37.5 -- not a known variable star
04:18:33.11 +75:10:21.0 -- not a known variable star
04:18:38.34 +71:09:35.9 -- a known variable star
04:19:51.22 +69:21:29.6 -- not a known variable star
04:21:41.67 +70:29:13.2 -- not a known variable star
04:22:03.16 +69:45:19.9 -- not a known variable star
04:22:24.45 +70:55:21.0 -- not a known variable star
04:23:24.12 +72:18:06.3 -- not a known variable star
04:24:04.67 +66:30:01.2 -- not a known variable star
04:24:09.29 +67:35:46.5 -- not a known variable star
04:24:42.66 +72:25:39.1 -- not a known variable star
04:25:18.52 +65:59:27.9 -- not a known variable star
04:28:22.35 +66:45:24.6 -- not a known variable star
04:28:30.63 +74:00:18.2 -- not a known variable star
04:29:15.52 +69:32:30.0 -- not a known variable star
04:31:03.65 +75:07:21.1 -- not a known variable star
04:33:55.15 +72:58:06.4 -- not a known variable star
04:34:51.47 +65:20:20.5 -- not a known variable star
04:35:14.65 +72:39:22.4 -- not a known variable star
04:37:27.18 +70:01:51.3 -- not a known variable star
04:39:50.40 +74:51:06.8 -- not a known variable star
04:41:24.56 +74:33:25.3 -- not a known variable star
04:41:58.65 +66:44:55.8 -- not a known variable star
04:42:42.89 +66:30:46.9 -- not a known variable star
04:44:10.25 +72:51:00.7 -- not a known variable star
04:45:23.36 +74:05:31.9 -- not a known variable star
04:46:22.00 +67:39:08.8 -- not a known variable star
04:46:33.85 +73:16:33.8 -- not a known variable star
04:46:34.74 +71:06:42.9 -- not a known variable star
04:47:22.82 +69:29:01.0 -- not a known variable star
04:50:00.75 +68:11:12.2 -- not a known variable star
04:50:49.70 +67:33:03.8 -- not a known variable star
04:51:43.05 +71:34:21.8 -- not a known variable star
04:53:12.29 +74:45:57.4 -- not a known variable star
04:53:15.02 +66:04:05.5 -- not a known variable star
04:54:27.37 +67:00:15.9 -- not a known variable star
04:55:43.67 +74:31:22.0 -- not a known variable star
04:56:59.57 +70:59:07.1 -- not a known variable star
04:57:20.82 +72:06:48.6 -- not a known variable star
04:59:20.59 +74:14:01.2 -- not a known variable star
05:00:02.55 +69:39:46.9 -- not a known variable star
05:00:10.82 +69:55:05.3 -- not a known variable star
05:02:22.38 +74:11:45.5 -- not a known variable star
05:03:02.46 +68:42:26.5 -- not a known variable star
05:05:06.66 +68:52:52.8 -- not a known variable star
05:05:46.98 +64:54:18.9 -- not a known variable star
05:06:17.22 +64:56:26.3 -- not a known variable star
05:06:41.68 +73:54:03.0 -- not a known variable star
05:07:14.96 +67:13:28.6 -- not a known variable star
05:09:03.89 +65:59:26.8 -- not a known variable star
05:10:28.79 +68:40:36.4 -- not a known variable star
05:11:09.00 +66:45:16.7 -- not a known variable star
05:12:16.44 +68:44:04.1 -- not a known variable star
05:12:16.81 +65:01:01.6 -- not a known variable star
05:12:37.45 +65:13:39.1 -- not a known variable star
05:12:59.65 +64:24:34.5 -- not a known variable star
05:13:57.33 +65:01:41.1 -- not a known variable star
05:15:10.02 +66:14:18.2 -- not a known variable star
05:15:21.85 +74:29:24.2 -- not a known variable star
05:15:22.19 +65:10:32.9 -- not a known variable star
05:15:27.03 +66:09:51.7 -- not a known variable star
05:16:25.50 +66:23:53.5 -- not a known variable star
05:16:41.61 +64:43:50.8 -- not a known variable star
05:17:26.62 +72:54:44.0 -- not a known variable star
05:17:29.91 +65:59:41.1 -- not a known variable star
05:17:35.34 +65:59:15.0 -- not a known variable star
05:17:39.82 +68:26:59.3 -- not a known variable star
05:18:08.92 +65:16:25.3 -- not a known variable star
05:18:42.89 +64:28:17.5 -- not a known variable star
05:18:43.49 +70:20:51.8 -- not a known variable star
05:19:13.84 +71:34:27.4 -- not a known variable star
05:20:09.63 +73:47:07.1 -- not a known variable star
05:21:14.20 +66:37:09.1 -- not a known variable star
05:21:31.94 +65:18:29.9 -- not a known variable star
05:21:58.18 +66:47:24.6 -- not a known variable star
05:22:00.12 +74:37:11.0 -- not a known variable star
05:22:13.44 +65:58:14.5 -- not a known variable star
05:23:17.38 +67:16:34.1 -- not a known variable star
05:23:33.40 +69:40:42.8 -- not a known variable star
05:25:28.11 +70:15:10.5 -- not a known variable star
05:25:43.87 +64:44:34.5 -- not a known variable star
05:28:27.35 +64:34:39.7 -- not a known variable star
05:30:25.09 +64:47:15.9 -- not a known variable star
05:31:25.84 +71:29:26.9 -- not a known variable star
05:32:24.37 +65:24:04.3 -- not a known variable star
05:32:37.99 +64:30:44.3 -- a known variable star
05:32:50.00 +66:05:09.2 -- not a known variable star
05:33:48.21 +66:47:42.0 -- not a known variable star
05:34:13.47 +70:20:39.4 -- not a known variable star
05:34:49.53 +72:44:22.1 -- not a known variable star
05:34:54.40 +70:02:21.4 -- not a known variable star
05:37:08.10 +66:12:52.0 -- not a known variable star
05:38:16.78 +64:18:56.6 -- not a known variable star
05:40:16.00 +63:55:28.2 -- not a known variable star
05:40:36.01 +64:27:57.7 -- not a known variable star
05:41:09.80 +66:39:24.1 -- not a known variable star
05:41:42.62 +63:30:22.8 -- not a known variable star
05:41:57.03 +66:34:14.8 -- not a known variable star
05:42:15.82 +69:41:59.5 -- not a known variable star
05:43:02.04 +70:23:05.6 -- not a known variable star
05:43:31.71 +64:09:08.8 -- not a known variable star
05:44:04.04 +71:24:17.1 -- not a known variable star
05:44:23.59 +65:05:29.3 -- not a known variable star
05:44:47.21 +68:01:36.2 -- not a known variable star
05:46:43.60 +65:00:07.8 -- not a known variable star
05:47:12.27 +66:16:41.8 -- not a known variable star
05:47:53.83 +71:31:06.9 -- not a known variable star
05:48:55.85 +67:06:40.2 -- not a known variable star
05:49:53.60 +71:43:25.7 -- not a known variable star
05:50:49.11 +70:34:50.0 -- a known variable star
05:51:40.97 +68:48:37.8 -- not a known variable star
05:51:45.16 +67:01:17.7 -- not a known variable star
05:52:38.21 +67:08:02.7 -- not a known variable star
05:52:49.78 +67:39:43.8 -- not a known variable star
05:53:49.36 +70:12:09.2 -- not a known variable star
05:54:21.34 +70:17:28.9 -- not a known variable star
05:54:25.48 +65:14:00.2 -- not a known variable star
05:57:27.66 +72:21:16.1 -- not a known variable star
05:57:57.38 +73:38:58.0 -- not a known variable star
05:58:28.34 +65:50:00.9 -- not a known variable star
05:59:18.39 +68:27:10.2 -- not a known variable star
05:59:36.27 +68:36:55.9 -- not a known variable star
05:59:39.99 +68:56:27.0 -- not a known variable star
06:01:31.71 +69:52:29.2 -- not a known variable star
06:02:29.07 +68:26:50.6 -- not a known variable star
06:02:36.92 +66:47:24.0 -- not a known variable star
06:03:05.64 +69:05:56.4 -- not a known variable star
06:03:11.95 +72:25:44.9 -- not a known variable star
06:05:34.61 +67:47:21.8 -- not a known variable star
06:07:43.54 +70:50:13.7 -- not a known variable star
06:08:03.56 +70:03:37.9 -- not a known variable star
06:08:58.95 +72:15:49.6 -- not a known variable star
06:09:37.39 +70:37:39.0 -- not a known variable star
06:10:22.43 +71:18:00.3 -- not a known variable star
06:12:48.34 +70:42:31.8 -- not a known variable star
06:15:50.95 +72:25:41.1 -- not a known variable star
06:16:48.34 +69:53:53.9 -- not a known variable star
06:22:44.78 +70:21:33.5 -- not a known variable star
06:31:27.42 +72:15:48.2 -- not a known variable star
06:31:57.25 +72:00:29.0 -- not a known variable star
06:32:01.43 +72:13:09.6 -- not a known variable star
Found 185 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
196 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 196 (excluding asteroids and hot pixels), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is 500
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Positions of planets computed with util/planet_finder/main.py for JD(UT)2461082.77180627 -observatory 500
22:36:06.59 -09:33:49.8 Mercury (-1.1mag)
22:13:05.83 -12:35:31.0 Venus (-3.9mag)
21:08:50.28 -17:31:45.4 Mars (1.1mag)
07:09:27.02 +22:48:02.0 Jupiter (-2.6mag)
00:00:59.26 -02:14:25.4 Saturn (1.0mag)
03:39:29.72 +19:19:52.2 Uranus (5.7mag)
00:02:22.08 -01:10:22.2 Neptune (7.8mag)
20:27:43.81 -23:02:56.0 Pluto (14.6mag)
16:34:48.65 -27:18:01.7 Moon (-9.9mag)
-rw-r--r-- 1 apache apache 362 Feb 11 00:35 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461082.77180627:
07:09:22.28 +22:48:14.0 Io (5.3mag)
07:09:34.32 +22:47:49.7 Europa (5.5mag)
07:09:37.57 +22:47:32.4 Ganymede (4.8mag)
07:09:45.72 +22:47:13.9 Callisto (6.0mag)
07:11:37.46 +23:08:40.2 Himalia (15.0mag)
07:09:24.15 +22:48:09.4 Thebe (15.8mag)
07:11:16.67 +23:10:51.9 Elara (17.0mag)
07:04:30.40 +24:01:37.5 Pasiphae (17.0mag)
07:18:27.92 +22:32:35.6 Carme (18.0mag)
00:00:58.46 -02:14:08.4 Titan (8.7mag)
00:00:55.67 -02:14:13.9 Rhea (10.0mag)
00:00:33.05 -02:16:07.5 Iapetus (11.5mag)
00:01:05.92 -02:14:15.3 Hyperion (14.7mag)
00:03:05.30 -02:00:58.6 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 11 00:35 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461082.77180627:
07:34:54.30 +22:41:20.1 JWST
20:15:08.46 -05:13:10.3 Chandra
07:58:26.45 -29:22:02.2 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 11 00:35 spacecraft.txt
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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)2461082.77180627 at 500
16:38:45.14 -10:49:28.5 17.8mag 10P/Tempel
03:28:12.38 +28:22:59.5 18.1mag 123P/West-Hartley
20:44:56.95 -10:24:00.6 22.4mag 141P/Machholz
00:57:27.57 +08:47:21.8 17.5mag 145P/Shoemaker-Levy 5
11:12:51.35 +29:08:27.0 17.8mag 164P/Christensen
09:39:21.88 -34:08:14.8 18.0mag 195P/Hill
15:50:40.53 -07:29:50.8 18.4mag 210P/Christensen
17:25:31.47 -21:36:38.4 17.4mag 218P/LINEAR
16:02:03.44 -18:17:17.7 15.2mag 235P/LINEAR
03:42:09.71 +25:39:02.3 17.5mag 240P/NEAT
15:00:57.24 +07:36:36.5 14.6mag 24P/Schaumasse
23:52:06.21 +04:05:04.6 18.0mag 261P/Larson
11:27:36.92 -03:36:44.7 17.4mag 29P/Schwassmann-Wachmann 1
01:06:12.22 +01:18:32.6 18.9mag 302P/Lemmon-PanSTARRS
07:07:06.75 +27:15:55.6 19.7mag 407P/PanSTARRS-Fuls
16:47:57.75 -11:17:58.8 17.5mag 40P/Vaisala 1
11:08:42.82 -09:17:17.6 16.6mag 43P/Wolf-Harrington
13:22:18.89 -05:02:31.8 19.4mag 489P/Denning
04:27:31.48 +49:30:00.4 17.7mag 493P/2024 Q2 (LONEOS)
06:02:44.19 +49:28:00.2 17.9mag 63P/Wild 1
22:53:12.78 -04:03:55.9 16.3mag 78P/Gehrels 2
19:20:34.83 -23:34:15.9 15.1mag 88P/Howell
15:21:21.47 -28:05:18.2 18.7mag P/2023 S1 (PanSTARRS)
04:43:19.43 -73:12:26.7 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:54.12 +31:10:56.4 18.1mag C/2017 K2 (PanSTARRS)
20:00:11.30 -64:55:02.7 18.1mag C/2020 V2 (ZTF)
17:16:35.18 +03:16:04.6 16.3mag C/2021 G2 (ATLAS)
22:45:21.66 +28:38:48.9 16.8mag C/2022 E2 (ATLAS)
03:27:38.79 +24:25:45.9 15.6mag C/2022 N2 (PANSTARRS)
09:12:14.98 +28:51:49.3 15.3mag C/2022 QE78 (ATLAS)
08:39:17.31 -07:51:23.3 16.6mag C/2022 R6 (PanSTARRS)
23:39:28.43 +48:05:03.7 17.9mag C/2023 C2 (ATLAS)
10:03:18.15 -22:12:51.2 17.5mag C/2023 F3 (ATLAS)
20:11:50.20 +61:17:54.4 17.2mag C/2023 H5 (Lemmon)
19:32:42.94 -03:16:52.2 16.1mag C/2023 R1 (PANSTARRS)
02:45:41.99 +35:48:04.5 18.5mag C/2023 RS61 (PanSTARRS)
20:41:35.26 +81:16:01.9 18.0mag C/2023 X2 (Lemmon)
06:57:18.28 +63:21:43.5 17.2mag C/2024 A1 (ATLAS)
00:20:43.71 -37:49:35.5 10.8mag C/2024 E1 (Wierzchos)
11:53:05.19 -04:33:05.3 18.1mag C/2024 G2 (ATLAS)
19:17:35.70 +00:19:43.2 19.0mag C/2024 G4 (PanSTARRS)
16:36:54.34 -03:03:40.7 17.8mag C/2024 G6 (ATLAS)
19:45:45.52 +01:21:09.3 15.7mag C/2024 J3 (ATLAS)
02:42:05.93 -33:38:25.0 15.4mag C/2024 T5 (ATLAS)
16:47:58.72 -53:58:08.2 15.2mag C/2025 A6 (Lemmon)
04:56:03.32 +66:38:13.5 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)
16:01:22.46 -20:48:32.2 15.0mag C/2025 L1 (ATLAS)
02:12:01.31 -17:27:37.5 16.6mag C/2025 Q3 (ATLAS)
01:55:37.47 +16:13:36.4 20.7mag C/2025 R2 (SWAN)
22:17:08.43 +17:32:50.3 16.8mag C/2025 R3 (PANSTARRS)
21:34:05.97 -14:27:29.2 20.3mag C/2025 T1 (ATLAS)
03:33:51.58 -25:34:28.2 17.5mag C/2026 A1 (MAPS)
20:22:07.62 +15:45:54.0 16.6mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.7K Feb 11 00:36 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
09:27:23.49 -32:00:30.90 SN 2023kuy 2026-01-21.16 15.43
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.41 -74:35:46.80 AT2026ahr 2026-01-20.09 16.98
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:24.99 +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
04:13:46.52 -05:02:18.30 ASASSN-26ad 2026-01-4.1 14.57
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
07:40:22.22 -10:00:59.30 AT2025aftz 2025-12-8.46 15.46
18:44:55.93 +47:57:37.60 ASASSN-25ez 2025-12-3.07 15.16
22:41:03.48 +38:58:01.90 ASASSN-25ey 2025-11-26.08 15.68
05:50:46.62 +58:54:53.50 SN 2025aedz 2025-11-24.25 16.66
06:35:50.19 -71:30:42.00 SN 2025adwn 2025-11-24.11 17.58
02:21:35.59 -14:18:04.90 AT2025aeft 2025-11-23.13 16.82
01:42:47.75 +12:31:45.10 AT2025aduf 2025-11-23.15 17.49
06:36:40.46 +33:18:26.10 ASASSN-25ev 2025-11-23.36 14.76
19:35:04.58 -21:08:37.40 ASASSN-25ex 2025-11-23.04 14.77
07:17:55.62 -09:26:55.10 ASASSN-25eu 2025-11-22.31 15.99
02:27:04.39 +55:22:14.40 ASASSN-25ew 2025-11-21.17 15.35
05:14:45.06 -14:26:58.00 SN 2025acrr 2025-11-20.08 17.05
23:07:18.85 +42:11:56.20 SN 2025acsn 2025-11-18.12 15.92
02:07:09.66 -09:01:32.00 SN2025acgk 2025-11-17.35 17.33
08:17:39.75 +04:36:51.80 AT 2025advo 2025-11-17.21 16.51
20:24:44.64 -50:23:02.20 SN 2025abnf 2025-11-16.03 15.61
04:22:41.06 -51:28:58.10 SN 2025aczu 2025-11-16.24 17.11
01:58:23.18 -29:19:37.10 AT 2025adsr 2025-11-16.07 17.18
02:15:50.04 -59:55:41.50 SN 2025acvj 2025-11-14.32 16.99
00:09:53.24 +03:36:48.20 SN 2025abuj 2025-11-14.09 16.79
13:28:48.71 +38:44:48.10 ASASSN-25et 2025-11-14.51 -2.76
-rw-r--r-- 1 apache apache 6.3K Feb 11 00:35 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:28.44 +41:18:24.5 TCP J00422844+4118245 2025-12-22.8736 18.5mag
16:42:59.22 +26:21:02.0 TCP J16425922+2621020 2025-12-26.8538 13.0mag
08:08:08.72 -19:48:46.5 TCP J08080872-1948465 2025-12-27.7904 16.66Cmag
00:42:58.48 +41:08:11.4 PNV J00425848+4108114 2025-12-28.7654 18.9mag
07:35:31.47 +09:10:34.1 TCP J07353147+0910341 2025-12-29.7527 14.77Cmag
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
-rw-r--r-- 1 apache apache 186K Feb 11 00:35 tocp_transients_list.txt