This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu
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,2461121.7819,11.12,0.05,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 20260322.2819 11.12CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:18:59.75 +64:31:42.7 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2819 2461121.7819 11.92 03:41:25.91 +72:39:20.4
134.90434 13.86488 galactic Cam Second-epoch detections are separated by 1.0" and 7.3 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 543597762796058368 | 03:41:19.09 +72:39:44.8 (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 543597762796058368,2461121.7819,11.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543597762796058368 20260322.2819 11.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:25.91 +72:39:20.4 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.09,0.05,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 20260322.2819 12.09CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:00.86 +68:10:46.4 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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 J0437484+693139,2461121.7819,12.26,0.05,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
NSVS J0437484+693139 20260322.2819 12.26CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:37:45.09 +69:31:52.6 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.32,0.05,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 20260322.2819 12.32CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:42:30.68 +66:40:53.4 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.27,0.05,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 20260322.2819 12.27CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:57:56.45 +70:12:50.7 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.32,0.05,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 20260322.2819 12.32CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:12:57.41 +67:27:58.1 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.31,0.05,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 20260322.2819 12.31CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:09:28.68 +68:58:24.5 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.32,0.05,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 20260322.2819 12.32CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:52:10.93 +69:04:38.8 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:41:07.85 +69:52:14.2 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.63,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:17:52.79 +74:21:04.3 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.45,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:12:01.38 +72:33:10.6 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.46,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:33:00.02 +69:49:58.2 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.31,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:20:19.20 +66:54:36.3 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.49,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:55:08.75 +72:15:43.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.41,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:08.14 +70:35:51.0 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.26,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:21:10.60 +68:13:26.2 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.32,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:39.72 +66:33:45.1 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.14,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:34:38.43 +66:07:05.0 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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 03 22.2819* 03 28 51.76 +73 05 52.8 13.1 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,2461121.7819,13.12,0.05,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 20260322.2819 13.12CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:28:51.76 +73:05:52.8 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.05,0.05,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 20260322.2819 13.05CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:13:42.88 +68:01:18.8 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:57:12.56 +65:29:17.0 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2819 2461121.7819 13.23 05:48:53.85 +65:55:44.9
147.41047 18.57231 galactic Cam Second-epoch detections are separated by 4.5" and 6.0 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 | 05:48:53.85 +65:55:44.9 (user input) | T | P | (position from user input) J-Ks=0.760+/-0.074 (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,2461121.7819,13.23,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:53.85 +65:55:44.9 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:14:28.53 +66:30:56.2 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.88,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 12.88CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:25:14.34 +68:40:28.5 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.64,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:37:14.57 +70:27:32.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,11.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 11.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:48.26 +70:34:25.8 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,11.85,0.05,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
target 20260322.2819 11.85CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:21.84 +65:57:48.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2819 2461121.7819 11.35 03:45:57.33 +68:00:23.7
138.16632 10.46014 galactic Cam Second-epoch detections are separated by 1.7" 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 | Gaia DR3 493476112928592512 | 03:45:59.00 +68:00:23.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 493476112928592512,2461121.7819,11.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493476112928592512 20260322.2819 11.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:57.33 +68:00:23.7 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,11.52,0.05,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 20260322.2819 11.52CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:47:15.74 +63:52:31.3 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,10.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 10.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:05.20 +67:18:04.9 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2819 2461121.7819 11.45 04:51:12.64 +68:13:48.0
142.33855 14.95970 galactic Cam Second-epoch detections are separated by 3.2" and 6.5 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 J072.7786+68.2306 | 04:51:12.64 +68:13:48.0 (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 J072.7786+68.2306,2461121.7819,11.45,0.05,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
ATO J072.7786+68.2306 20260322.2819 11.45CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:51:12.64 +68:13:48.0 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,11.65,0.05,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 20260322.2819 11.65CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:01.15 +66:43:18.2 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2819 2461121.7819 11.61 04:51:11.37 +68:13:32.8
142.34081 14.95559 galactic Cam Second-epoch detections are separated by 2.8" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J072.7786+68.2306 | 04:51:11.37 +68:13:32.8 (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 J072.7786+68.2306,2461121.7819,11.61,0.05,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
ATO J072.7786+68.2306 20260322.2819 11.61CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:51:11.37 +68:13:32.8 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2819 2461121.7819 11.61 04:42:00.42 +69:05:12.2
141.10659 14.82799 galactic Cam Second-epoch detections are separated by 2.6" and 6.8 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 495938675378981376 | 04:42:03.83 +69:05:36.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 495938675378981376,2461121.7819,11.61,0.05,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
Gaia DR3 495938675378981376 20260322.2819 11.61CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:42:00.42 +69:05:12.2 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,11.89,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:07.65 +67:38:39.4 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,11.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 11.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:45:32.04 +75:04:38.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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 J0418017+711356,2461121.7819,11.95,0.05,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
NSVS J0418017+711356 20260322.2819 11.95CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:18:00.36 +71:14:00.4 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 12.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:25:17.07 +70:15:54.2 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.26,0.05,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 20260322.2819 12.26CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:24.12 +68:08:34.9 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.16,0.05,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 20260322.2819 12.16CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:31:25.46 +71:29:08.7 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.46,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:37:03.89 +74:14:30.2 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.45,0.05,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 20260322.2819 12.45CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:25:27.56 +70:14:50.0 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2819 2461121.7819 12.43 05:49:30.84 +65:53:52.6
147.46853 18.61591 galactic Cam Second-epoch detections are separated by 6.1" and 6.0 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 | 05:49:30.84 +65:53:52.6 (user input) | T | P | (position from user input) J-Ks=0.408+/-0.073 (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,2461121.7819,12.43,0.05,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 20260322.2819 12.43CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:49:30.84 +65:53:52.6 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.48,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:01.72 +68:05:45.7 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.54,0.05,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 20260322.2819 12.54CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:21.25 +68:02:16.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.56,0.05,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
target 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:16:19.61 +73:33:58.6 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.47,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:24.56 +68:22:02.2 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 12.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:08.71 +66:13:46.9 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.40,0.05,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 20260322.2819 12.40CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:10:07.33 +68:21:09.6 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.54,0.05,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 20260322.2819 12.54CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:51.44 +64:05:50.8 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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 03 22.2819* 03 29 06.52 +72 34 22.7 12.5 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,2461121.7819,12.51,0.05,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 20260322.2819 12.51CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:29:06.52 +72:34:22.7 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2819 2461121.7819 12.54 04:27:17.52 +71:47:20.3
138.14598 15.63549 galactic Cam Second-epoch detections are separated by 5.4" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 500429214005075328 | 04:27:22.92 +71:47:49.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 500429214005075328,2461121.7819,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 500429214005075328 20260322.2819 12.54CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:27:17.52 +71:47:20.3 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.73,0.05,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 20260322.2819 12.73CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:20:50.62 +66:51:55.2 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.66,0.05,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 20260322.2819 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:07.29 +70:08:05.5 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2819 2461121.7819 12.58 03:57:22.41 +71:25:04.5
136.69225 13.70560 galactic Cam Second-epoch detections are separated by 3.6" 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 | Gaia DR3 495284156721043456 | 03:57:27.88 +71:25:33.1 (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 495284156721043456,2461121.7819,12.58,0.05,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
Gaia DR3 495284156721043456 20260322.2819 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:57:22.41 +71:25:04.5 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.64,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:54:12.65 +66:30:04.1 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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 495750899407105536,2461121.7819,12.62,0.05,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
Gaia DR3 495750899407105536 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:59.25 +67:44:49.8 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.77,0.05,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 20260322.2819 12.77CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:43:11.16 +64:40:38.6 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2819 2461121.7819 12.70 04:51:09.10 +68:10:39.5
142.37833 14.92372 galactic Cam Second-epoch detections are separated by 4.5" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ST Cam | 04:51:13.34 +68:10:07.6 (Gaia DR3) | SRB (local) | : (local) | Gaia3var=VARIABLE SpType: C 1869AN.....73..129S ST Cam
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
ST Cam,2461121.7819,12.70,0.05,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
ST Cam 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:51:09.10 +68:10:39.5 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.69,0.05,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 20260322.2819 12.69CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:04.98 +68:14:45.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2819 2461121.7819 12.97 06:15:28.90 +71:02:58.6
143.28022 22.71272 galactic Cam Second-epoch detections are separated by 4.4" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 1107565000693781760 | 06:15:32.98 +71:03:29.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 1107565000693781760,2461121.7819,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1107565000693781760 20260322.2819 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:15:28.90 +71:02:58.6 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.73,0.05,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 20260322.2819 12.73CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:03.71 +66:29:44.6 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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 03 22.2819* 03 34 58.15 +71 38 57.5 12.7 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
Gaia DR3 543153422658023040,2461121.7819,12.74,0.05,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
Gaia DR3 543153422658023040 20260322.2819 12.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:34:58.15 +71:38:57.5 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:16.16 +67:46:27.8 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2819 2461121.7819 12.63 03:37:04.95 +69:37:38.9
136.51057 11.25047 galactic Cas Second-epoch detections are separated by 0.8" 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 | Gaia DR3 494616272126777600 | 03:36:56.34 +69:37:42.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: K0 1956PMcCO..13a....B AG+69 162
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 03 22.2819* 03 37 04.95 +69 37 38.9 12.6 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
Gaia DR3 494616272126777600,2461121.7819,12.63,0.05,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
Gaia DR3 494616272126777600 20260322.2819 12.63CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:04.95 +69:37:38.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:39:51.44 +74:51:08.9 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:00.47 +72:50:48.4 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.98,0.05,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
target 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:48:44.31 +66:46:18.3 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.94,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:02:22.93 +65:05:21.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:13:15.58 +66:08:29.9 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.99,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 12.99CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:55:08.26 +66:57:32.4 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.08,0.05,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 20260322.2819 13.08CV 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:22:42.85 +70:21:08.4 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.97,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 12.97CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:30:26.64 +69:08:36.1 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 13.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:32:49.67 +63:53:44.8 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:16:53.31 +69:09:51.9 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.00,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:45:00.00 +75:04:04.7 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.09,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:59:20.89 +74:13:58.3 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.32,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:27:12.08 +70:25:51.6 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.29,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:53.59 +67:06:07.5 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.15,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:06.43 +70:35:19.8 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.14,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:57:27.41 +68:33:28.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.23,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:26.55 +72:22:32.8 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2819 2461121.7819 13.22 04:38:23.18 +65:27:17.1
143.75176 12.23948 galactic Cam Second-epoch detections are separated by 3.0" 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 483028209845147904 | 04:38:29.75 +65:27:07.7 (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 483028209845147904,2461121.7819,13.22,0.05,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 483028209845147904 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:38:23.18 +65:27:17.1 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.48,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:47.83 +67:39:12.3 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.34,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:17:27.94 +71:50:59.3 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:25:41.83 +64:43:56.3 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2819 2461121.7819 13.34 04:33:42.86 +69:30:55.3
140.28125 14.53958 galactic Cam Second-epoch detections are separated by 5.9" 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 | Gaia DR3 496761006995740800 | 04:33:43.28 +69:31:26.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 496761006995740800,2461121.7819,13.34,0.05,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
Gaia DR3 496761006995740800 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:33:42.86 +69:30:55.3 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:44:30.23 +71:55:32.0 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2819 2461121.7819 13.35 05:00:30.01 +70:04:35.1
141.28778 16.71160 galactic Cam Second-epoch detections are separated by 5.1" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 496435375456780160 | 05:00:34.55 +70:04:50.2 (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 496435375456780160,2461121.7819,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 496435375456780160 20260322.2819 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:00:30.01 +70:04:35.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.41,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:23:58.93 +71:53:36.1 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 13.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:59.54 +70:21:41.5 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.37,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:22:57.96 +71:37:39.1 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.38,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:01:19.00 +71:44:34.6 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.73,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:23:30.24 +71:26:15.5 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.59,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:00:06.41 +74:34:47.1 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.38,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:59:25.51 +73:46:14.7 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.62,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:33.33 +68:08:08.1 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.52,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:19.71 +70:17:04.7 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 13.42CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:45:07.48 +74:15:01.9 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.54,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:20:14.92 +64:10:29.6 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.46,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:37:39.68 +68:10:37.6 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.34,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:47:24.76 +69:28:47.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:35.93 +67:07:30.8 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.62,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:31:24.90 +72:15:28.1 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:57:56.91 +73:38:45.0 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.66,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:09.91 +73:35:27.0 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.40,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:13:17.24 +70:20:12.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.49,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:31:33.34 +74:01:54.2 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.75,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:33:31.17 +71:47:37.8 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.54,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:12:00.38 +69:32:15.5 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:12:17.48 +70:34:57.0 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.57,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:44:33.84 +63:52:14.3 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2819 2461121.7819 13.56 05:47:10.04 +66:16:05.9
147.00797 18.55965 galactic Cam Second-epoch detections are separated by 5.5" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ASASSN-V J054712.61+661534.1 | 05:47:12.61 +66:15:34.0 (Gaia DR3) | ROT (local) | 2458118.58900 (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 J054712.61+661534.1,2461121.7819,13.56,0.05,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
ASASSN-V J054712.61+661534.1 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:47:10.04 +66:16:05.9 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.53,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:39:36.65 +67:55:23.6 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:53.64 +69:24:30.3 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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 481230370895616256,2461121.7819,13.64,0.05,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
Gaia DR3 481230370895616256 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:28.21 +67:10:34.7 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.64,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:46:30.23 +70:37:03.2 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.72,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:10.68 +72:25:25.2 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 13.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:59:33.29 +74:03:12.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.61,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:55:44.87 +71:26:46.8 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.64,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:55:44.34 +74:31:21.0 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:28:51.13 +69:13:48.5 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.68,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:19.83 +70:27:54.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.77,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:28:29.50 +70:27:41.7 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.70,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:36:45.86 +72:15:20.8 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2819 2461121.7819 13.60 05:04:12.63 +70:10:54.8
141.38207 17.03158 galactic Cam Second-epoch detections are separated by 3.8" and 6.4 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 496431153506868352 | 05:04:19.33 +70:10:47.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 496431153506868352,2461121.7819,13.60,0.05,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
Gaia DR3 496431153506868352 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:04:12.63 +70:10:54.8 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:02:06.77 +73:08:34.6 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.64,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:00:58.15 +64:59:07.5 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.57,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:09.81 +67:08:23.9 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.55,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:55:40.07 +69:53:38.1 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.49,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:55:51.64 +66:08:49.5 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.65,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:51:56.19 +69:41:16.1 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.69,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:06:15.77 +64:55:52.5 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:41:06.02 +70:59:16.6 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,13.78,0.05,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 20260322.2819 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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:17:21.77 +72:57:07.1 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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,2461121.7819,12.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2819 12.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:30:42.74 +64:21:05.7 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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+661955,2461121.7819,11.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0405390+661955 20260322.2819 11.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:05:37.89 +66:19:58.3 ;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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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_2026-03-22_01-46-18_20_00sec_-14_90C_LIGHT_0134_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_2026-03-22_01-45-16_20_00sec_-14_90C_LIGHT_0133_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: 2461121.78227069 22.03.2026 06:46:18.188 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 11
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: 4 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): 15757
Objects passed selection criteria: 15745
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: 15153.2
Average stars matched: 14828 (97.8536 %)
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 Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 01:49:32 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.82849338 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: 2461121.78227069 22.03.2026 06:46:18.188 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 159
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): 108750
Objects passed selection criteria: 108520
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 103570
Average stars matched: 100240 (96.785 %)
Memory usage VmPeak: 1892488 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 02:01:43 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.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: 2461121.78155735
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_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_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits'
wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.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 04:47:58.883 +70:00:17.33
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:47:48.196 +70:00:29.12
Second-epoch image center 04:47:57.386 +70:00:56.15
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 04:47:58.883 +70:00:17.33
Second-epoch second image center 04:47:57.386 +70:00:56.15
Angular distance between the image centers 0.01099 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.jpgnzJtbJP
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.MHNzk5gZyu
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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits &> /tmp/tmp.y7Ol3Vcejq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits &> /tmp/tmp.iNJfz7AmDz
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.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.
The calibration function type and coefficients are written to calib.txt_param
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
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 10 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix 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_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
2.1 pix fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.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
15.0 mag. fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
15.0 mag. fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
All-image limiting magnitude estimate: 15.0 (SNR ) 12.1 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.jpgnzJtbJP (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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/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.MHNzk5gZyu (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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/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.y7Ol3Vcejq (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
Checking if the catalog wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.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_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
WCS catalog name: wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=937, passed=14321
Got 14321 stars (including 13366 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits.cat
util/solve_plate_with_UCAC5 got 14321 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.5'
Seting catalog search parameters based on the expected field of view 931.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012937 (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 0.010350 (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 271 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: 6.88"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.81"
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 333 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.60"
Estimated accuracy of the plate solution: 5.84"
Excluding outliers - 304 stars left (next iteration limit 236)
The image catalog is written to wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits -region wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.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.iNJfz7AmDz (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
Checking if the catalog wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.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_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
WCS catalog name: wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=951, passed=14260
Got 14260 stars (including 13289 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits.cat
util/solve_plate_with_UCAC5 got 14260 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.5'
Seting catalog search parameters based on the expected field of view 931.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012937 (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 0.010350 (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 266 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: 6.90"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.70"
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 330 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.60"
Estimated accuracy of the plate solution: 5.66"
Excluding outliers - 303 stars left (next iteration limit 235)
The image catalog is written to wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits -region wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits'
Saving fully-calibrated image wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits'
Saving fully-calibrated image wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits'
Saving fully-calibrated image wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits'
Preparing the HTML report for the field Cam-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21076.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out21051.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21089.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21100.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out21114.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 21s
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: 6s
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Considering the candidate 21051_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 21051_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 21076_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 21076_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 did not pass the final checks
**** FOUND 04:33:19.11 +70:27:44.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.80, MAG_FAINT_SEARCH_LIMIT=12.78)GAIADR2_OUTPUT=# 4.522 497068251776071296 068.33335138020 +70.46251921137 11.6749 10.9767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.522#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21081_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 21081_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 21089_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 21089_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 21096_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 21096_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 21100_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 21100_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 21101_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 21101_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 21102_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 21102_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21104_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 21104_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 21114_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 21114_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
make_report_in_HTML.sh Phase 2 (HTML assembly): 1s
make_report_in_HTML.sh TOTAL: 28s
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 ####
05:18:59.75 +64:31:42.7
03:41:25.91 +72:39:20.4
04:50:00.86 +68:10:46.4
04:37:45.09 +69:31:52.6
05:42:30.68 +66:40:53.4
04:57:56.45 +70:12:50.7
05:12:57.41 +67:27:58.1
05:09:28.68 +68:58:24.5
04:52:10.93 +69:04:38.8
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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.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_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.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_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits exists and is non-empty
wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.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 04:47:58.883 +70:00:17.33
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:47:48.196 +70:00:29.12
Second-epoch image center 04:47:57.386 +70:00:56.15
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 04:47:58.883 +70:00:17.33
Second-epoch second image center 04:47:57.386 +70:00:56.15
Angular distance between the image centers 0.01099 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.AgKt9xItKq
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.b0lcMptkyk
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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits &> /tmp/tmp.hiuMxTSuyE
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits &> /tmp/tmp.0P4S9v8Wph
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.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.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.485424
a=0.000000 b=1.000000 c=21.485424
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
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 146 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
2.1 pix fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
2.1 pix fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.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
13.9 mag. fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
13.9 mag. fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.3 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.AgKt9xItKq (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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/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.b0lcMptkyk (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_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/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.hiuMxTSuyE (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
Checking if the catalog wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.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_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
WCS catalog name: wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=12, blended=6749, passed=94951
Got 94951 stars (including 88053 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits.cat
util/solve_plate_with_UCAC5 got 94951 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.5'
Seting catalog search parameters based on the expected field of view 931.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012937 (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 0.010350 (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 275 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: 7.00"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.65"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 332 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.63"
Estimated accuracy of the plate solution: 5.75"
Excluding outliers - 301 stars left (next iteration limit 235)
The image catalog is written to wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits -region wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.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.0P4S9v8Wph (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
Checking if the catalog wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.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_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
WCS catalog name: wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=15, blended=6789, passed=95347
Got 95347 stars (including 88408 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits.cat
util/solve_plate_with_UCAC5 got 95347 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.5'
Seting catalog search parameters based on the expected field of view 931.5 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012937 (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 0.010350 (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 275 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: 7.08"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 7.01"
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 332 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.97"
Estimated accuracy of the plate solution: 5.92"
Excluding outliers - 305 stars left (next iteration limit 240)
The image catalog is written to wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits -region wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Saving fully-calibrated image wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Saving fully-calibrated image wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-45-16_20.00sec_-14.90C_LIGHT_0133.fits
Saving fully-calibrated image wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q1b1x1_014656_TTUQ1b1x1_9502_OHJQImmu/wcs_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134.fits
Preparing the HTML report for the field Cam-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out132962.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out132944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132978.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132991.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132997.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133008.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133011.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133020.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133080.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133184.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133233.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133255.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133286.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133287.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133349.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133359.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133362.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133388.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133397.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133401.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133428.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133433.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133442.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133446.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133472.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133482.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133492.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133498.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133500.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133504.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133520.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133531.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133541.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133558.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133606.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133632.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133636.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133675.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133687.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133688.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133705.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133709.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133728.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133731.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133752.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133794.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133801.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133804.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133811.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133812.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133823.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133873.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133899.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133914.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133934.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133939.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134068.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134084.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134096.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134104.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134117.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134120.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134162.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134170.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134172.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134194.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134219.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134229.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134251.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134261.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134262.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134301.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134312.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134313.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134328.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134342.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out74637.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): 193s
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: 83s
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Considering the candidate 132944_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 132944_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 132950_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 132950_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 132953_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 132953_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 132960_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 132960_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 132962_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 132962_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 did not pass the final checks
**** FOUND 04:01:51.72 +71:49:40.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 3.571 495320440604246272 060.46322646623 +71.82855486140 14.4459 13.8281 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.571#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132964_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 132964_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 132970_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 132970_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 did not pass the final checks
Rejecting candidate due to large distance (11.9") between the two second-epoch detections
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Considering the candidate 132973_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 132973_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 132978_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 132978_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 132981_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 132981_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 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 132986_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 132986_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 132991_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 132991_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 132994_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 132994_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 132996_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 132996_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 132997_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 132997_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133001_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133001_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133007_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133007_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133008_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133008_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133009_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133009_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133011_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133011_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133013_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133013_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133016_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133016_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133018_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133018_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133019_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133019_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133020_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133020_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133080_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133080_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133141_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133141_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133160_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 133160_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 did not pass the final checks
**** FOUND 04:13:40.36 +72:09:28.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 133170_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133170_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133182_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133182_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133184_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133184_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133233_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133233_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133255_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133255_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133261_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133261_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133262_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133262_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133286_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133286_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133287_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133287_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133340_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 133340_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 did not pass the final checks
Rejecting candidate due to large distance (20.3") between the two second-epoch detections
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Considering the candidate 133349_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133349_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133359_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133359_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133362_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133362_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133365_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133365_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133388_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133388_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133397_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133397_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133401_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133401_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133406_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133406_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133427_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133427_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133428_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133428_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133433_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133433_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133442_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133442_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133444_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 133444_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 133446_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133446_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133455_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 133455_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 did not pass the final checks
**** FOUND 04:20:25.81 +65:08:25.5 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 133472_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133472_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133482_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133482_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133491_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 133491_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 133492_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133492_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133498_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133498_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133500_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133500_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133504_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133504_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133507_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133507_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133520_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133520_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133531_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133531_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133541_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133541_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133550_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133550_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133555_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 133555_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 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 133558_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133558_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133574_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133574_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133606_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133606_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133632_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133632_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133636_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133636_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133639_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133639_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133675_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133675_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133681_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133681_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133687_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133687_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133688_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133688_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133705_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133705_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133706_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133706_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133709_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133709_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133728_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133728_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133731_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133731_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133739_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133739_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133752_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133752_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133794_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133794_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133801_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133801_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133802_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133802_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133804_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133804_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133811_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133811_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133812_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133812_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133823_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133823_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133841_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133841_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133867_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133867_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133873_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133873_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133899_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133899_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133907_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 133907_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 did not pass the final checks
Rejecting candidate due to large distance (10.3") between the two second-epoch detections
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Considering the candidate 133914_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133914_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133921_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133921_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133930_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133930_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133934_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133934_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133939_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133939_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133957_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133957_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133973_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133973_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133976_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 133976_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 133990_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133990_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 133992_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 133992_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 did not pass the final checks
Rejecting candidate due to large distance (18.7") between the two second-epoch detections
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Considering the candidate 133996_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 133996_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 134003_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134003_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 134005_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134005_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 134009_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134009_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134032_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 134032_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 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 134064_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134064_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
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Considering the candidate 134068_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134068_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134076_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134076_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134084_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134084_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134096_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134096_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134104_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134104_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134117_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134117_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134120_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134120_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134136_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134136_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134142_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134142_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134147_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 134147_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 did not pass the final checks
Rejecting candidate due to large distance (9.6") between the two second-epoch detections
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Considering the candidate 134148_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134148_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134151_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134151_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134157_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134157_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134158_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 134158_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 did not pass the final checks
Rejecting candidate due to large distance (9.4") between the two second-epoch detections
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Considering the candidate 134162_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134162_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134168_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134168_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134170_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134170_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134172_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134172_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134194_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134194_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134212_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134212_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134219_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134219_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134229_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134229_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134251_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134251_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134261_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134261_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134262_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134262_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134284_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134284_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134301_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134301_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134312_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134312_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134313_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134313_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134328_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134328_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134342_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134342_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134366_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 134366_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 72928_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
The candidate 72928_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134 did not pass the final checks
**** FOUND 05:18:59.37 +64:31:45.6 in the exclusion list exclusion_list_local.txt ****
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Considering the candidate 74637_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 74637_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90043_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
Preparing report for the candidate 90043_fd_Cam-06-Q1b1x1_2026-03-22_01-46-18_20.00sec_-14.90C_LIGHT_0134
make_report_in_HTML.sh Phase 2 (HTML assembly): 19s
make_report_in_HTML.sh TOTAL: 295s
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 ####
05:18:59.75 +64:31:42.7
03:41:25.91 +72:39:20.4
04:50:00.86 +68:10:46.4
04:37:45.09 +69:31:52.6
05:42:30.68 +66:40:53.4
04:57:56.45 +70:12:50.7
05:12:57.41 +67:27:58.1
05:09:28.68 +68:58:24.5
04:52:10.93 +69:04:38.8
04:41:07.85 +69:52:14.2
04:17:52.79 +74:21:04.3
04:12:01.38 +72:33:10.6
04:33:00.02 +69:49:58.2
05:20:19.20 +66:54:36.3
04:55:08.75 +72:15:43.3
04:24:08.14 +70:35:51.0
05:21:10.60 +68:13:26.2
05:59:39.72 +66:33:45.1
04:34:38.43 +66:07:05.0
03:28:51.76 +73:05:52.8
04:13:42.88 +68:01:18.8
04:57:12.56 +65:29:17.0
05:48:53.85 +65:55:44.9
04:14:28.53 +66:30:56.2
05:25:14.34 +68:40:28.5
05:37:14.57 +70:27:32.7
05:50:48.26 +70:34:25.8
05:55:21.84 +65:57:48.7
03:45:57.33 +68:00:23.7
05:47:15.74 +63:52:31.3
05:29:05.20 +67:18:04.9
04:51:12.64 +68:13:48.0
05:57:01.15 +66:43:18.2
04:51:11.37 +68:13:32.8
04:42:00.42 +69:05:12.2
04:50:07.65 +67:38:39.4
04:45:32.04 +75:04:38.3
04:18:00.36 +71:14:00.4
05:25:17.07 +70:15:54.2
05:58:24.12 +68:08:34.9
05:31:25.46 +71:29:08.7
05:37:03.89 +74:14:30.2
05:25:27.56 +70:14:50.0
05:49:30.84 +65:53:52.6
05:50:01.72 +68:05:45.7
05:55:21.25 +68:02:16.3
05:16:19.61 +73:33:58.6
05:03:24.56 +68:22:02.2
05:15:08.71 +66:13:46.9
04:10:07.33 +68:21:09.6
05:29:51.44 +64:05:50.8
03:29:06.52 +72:34:22.7
04:27:17.52 +71:47:20.3
05:20:50.62 +66:51:55.2
04:50:07.29 +70:08:05.5
03:57:22.41 +71:25:04.5
04:54:12.65 +66:30:04.1
04:26:59.25 +67:44:49.8
05:43:11.16 +64:40:38.6
04:51:09.10 +68:10:39.5
04:24:04.98 +68:14:45.8
06:15:28.90 +71:02:58.6
04:24:03.71 +66:29:44.6
03:34:58.15 +71:38:57.5
06:03:16.16 +67:46:27.8
03:37:04.95 +69:37:38.9
04:39:51.44 +74:51:08.9
04:56:00.47 +72:50:48.4
04:48:44.31 +66:46:18.3
05:02:22.93 +65:05:21.9
05:13:15.58 +66:08:29.9
04:55:08.26 +66:57:32.4
06:22:42.85 +70:21:08.4
04:30:26.64 +69:08:36.1
05:32:49.67 +63:53:44.8
04:16:53.31 +69:09:51.9
04:45:00.00 +75:04:04.7
04:59:20.89 +74:13:58.3
05:27:12.08 +70:25:51.6
05:48:53.59 +67:06:07.5
05:15:06.43 +70:35:19.8
04:57:27.41 +68:33:28.0
06:25:26.55 +72:22:32.8
04:38:23.18 +65:27:17.1
05:52:47.83 +67:39:12.3
06:17:27.94 +71:50:59.3
05:25:41.83 +64:43:56.3
04:33:42.86 +69:30:55.3
05:44:30.23 +71:55:32.0
05:00:30.01 +70:04:35.1
06:23:58.93 +71:53:36.1
04:49:59.54 +70:21:41.5
05:22:57.96 +71:37:39.1
05:01:19.00 +71:44:34.6
06:23:30.24 +71:26:15.5
05:00:06.41 +74:34:47.1
03:59:25.51 +73:46:14.7
06:01:33.33 +68:08:08.1
05:54:19.71 +70:17:04.7
04:45:07.48 +74:15:01.9
05:20:14.92 +64:10:29.6
04:37:39.68 +68:10:37.6
04:47:24.76 +69:28:47.6
05:52:35.93 +67:07:30.8
06:31:24.90 +72:15:28.1
05:57:56.91 +73:38:45.0
05:50:09.91 +73:35:27.0
05:13:17.24 +70:20:12.0
05:31:33.34 +74:01:54.2
06:33:31.17 +71:47:37.8
04:12:00.38 +69:32:15.5
06:12:17.48 +70:34:57.0
05:44:33.84 +63:52:14.3
05:47:10.04 +66:16:05.9
04:39:36.65 +67:55:23.6
05:46:53.64 +69:24:30.3
05:34:28.21 +67:10:34.7
04:46:30.23 +70:37:03.2
06:03:10.68 +72:25:25.2
04:59:33.29 +74:03:12.1
03:55:44.87 +71:26:46.8
04:55:44.34 +74:31:21.0
05:28:51.13 +69:13:48.5
04:25:19.83 +70:27:54.6
05:28:29.50 +70:27:41.7
04:36:45.86 +72:15:20.8
05:04:12.63 +70:10:54.8
05:02:06.77 +73:08:34.6
05:00:58.15 +64:59:07.5
04:24:09.81 +67:08:23.9
04:55:40.07 +69:53:38.1
03:55:51.64 +66:08:49.5
04:51:56.19 +69:41:16.1
05:06:15.77 +64:55:52.5
04:41:06.02 +70:59:16.6
04:17:21.77 +72:57:07.1
05:30:42.74 +64:21:05.7
04:05:37.89 +66:19:58.3
########### 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 ####
05:18:59.75 +64:31:42.7
03:41:25.91 +72:39:20.4
04:50:00.86 +68:10:46.4
04:37:45.09 +69:31:52.6
05:42:30.68 +66:40:53.4
04:57:56.45 +70:12:50.7
05:12:57.41 +67:27:58.1
05:09:28.68 +68:58:24.5
04:52:10.93 +69:04:38.8
04:41:07.85 +69:52:14.2
04:17:52.79 +74:21:04.3
04:12:01.38 +72:33:10.6
04:33:00.02 +69:49:58.2
05:20:19.20 +66:54:36.3
04:55:08.75 +72:15:43.3
04:24:08.14 +70:35:51.0
05:21:10.60 +68:13:26.2
05:59:39.72 +66:33:45.1
04:34:38.43 +66:07:05.0
03:28:51.76 +73:05:52.8
04:13:42.88 +68:01:18.8
04:57:12.56 +65:29:17.0
05:48:53.85 +65:55:44.9
04:14:28.53 +66:30:56.2
05:25:14.34 +68:40:28.5
05:37:14.57 +70:27:32.7
05:50:48.26 +70:34:25.8
05:55:21.84 +65:57:48.7
03:45:57.33 +68:00:23.7
05:47:15.74 +63:52:31.3
05:29:05.20 +67:18:04.9
04:51:12.64 +68:13:48.0
05:57:01.15 +66:43:18.2
04:51:11.37 +68:13:32.8
04:42:00.42 +69:05:12.2
04:50:07.65 +67:38:39.4
04:45:32.04 +75:04:38.3
04:18:00.36 +71:14:00.4
05:25:17.07 +70:15:54.2
05:58:24.12 +68:08:34.9
05:31:25.46 +71:29:08.7
05:37:03.89 +74:14:30.2
05:25:27.56 +70:14:50.0
05:49:30.84 +65:53:52.6
05:50:01.72 +68:05:45.7
05:55:21.25 +68:02:16.3
05:16:19.61 +73:33:58.6
05:03:24.56 +68:22:02.2
05:15:08.71 +66:13:46.9
04:10:07.33 +68:21:09.6
05:29:51.44 +64:05:50.8
03:29:06.52 +72:34:22.7
04:27:17.52 +71:47:20.3
05:20:50.62 +66:51:55.2
04:50:07.29 +70:08:05.5
03:57:22.41 +71:25:04.5
04:54:12.65 +66:30:04.1
04:26:59.25 +67:44:49.8
05:43:11.16 +64:40:38.6
04:51:09.10 +68:10:39.5
04:24:04.98 +68:14:45.8
06:15:28.90 +71:02:58.6
04:24:03.71 +66:29:44.6
03:34:58.15 +71:38:57.5
06:03:16.16 +67:46:27.8
03:37:04.95 +69:37:38.9
04:39:51.44 +74:51:08.9
04:56:00.47 +72:50:48.4
04:48:44.31 +66:46:18.3
05:02:22.93 +65:05:21.9
05:13:15.58 +66:08:29.9
04:55:08.26 +66:57:32.4
06:22:42.85 +70:21:08.4
04:30:26.64 +69:08:36.1
05:32:49.67 +63:53:44.8
04:16:53.31 +69:09:51.9
04:45:00.00 +75:04:04.7
04:59:20.89 +74:13:58.3
05:27:12.08 +70:25:51.6
05:48:53.59 +67:06:07.5
05:15:06.43 +70:35:19.8
04:57:27.41 +68:33:28.0
06:25:26.55 +72:22:32.8
04:38:23.18 +65:27:17.1
05:52:47.83 +67:39:12.3
06:17:27.94 +71:50:59.3
05:25:41.83 +64:43:56.3
04:33:42.86 +69:30:55.3
05:44:30.23 +71:55:32.0
05:00:30.01 +70:04:35.1
06:23:58.93 +71:53:36.1
04:49:59.54 +70:21:41.5
05:22:57.96 +71:37:39.1
05:01:19.00 +71:44:34.6
06:23:30.24 +71:26:15.5
05:00:06.41 +74:34:47.1
03:59:25.51 +73:46:14.7
06:01:33.33 +68:08:08.1
05:54:19.71 +70:17:04.7
04:45:07.48 +74:15:01.9
05:20:14.92 +64:10:29.6
04:37:39.68 +68:10:37.6
04:47:24.76 +69:28:47.6
05:52:35.93 +67:07:30.8
06:31:24.90 +72:15:28.1
05:57:56.91 +73:38:45.0
05:50:09.91 +73:35:27.0
05:13:17.24 +70:20:12.0
05:31:33.34 +74:01:54.2
06:33:31.17 +71:47:37.8
04:12:00.38 +69:32:15.5
06:12:17.48 +70:34:57.0
05:44:33.84 +63:52:14.3
05:47:10.04 +66:16:05.9
04:39:36.65 +67:55:23.6
05:46:53.64 +69:24:30.3
05:34:28.21 +67:10:34.7
04:46:30.23 +70:37:03.2
06:03:10.68 +72:25:25.2
04:59:33.29 +74:03:12.1
03:55:44.87 +71:26:46.8
04:55:44.34 +74:31:21.0
05:28:51.13 +69:13:48.5
04:25:19.83 +70:27:54.6
05:28:29.50 +70:27:41.7
04:36:45.86 +72:15:20.8
05:04:12.63 +70:10:54.8
05:02:06.77 +73:08:34.6
05:00:58.15 +64:59:07.5
04:24:09.81 +67:08:23.9
04:55:40.07 +69:53:38.1
03:55:51.64 +66:08:49.5
04:51:56.19 +69:41:16.1
05:06:15.77 +64:55:52.5
04:41:06.02 +70:59:16.6
04:17:21.77 +72:57:07.1
05:30:42.74 +64:21:05.7
04:05:37.89 +66:19:58.3
###################################################################################
05:18:59.75 +64:31:42.7 -- not an asteroid (will add it to exclusion list)
03:41:25.91 +72:39:20.4 -- not an asteroid (will add it to exclusion list)
04:50:00.86 +68:10:46.4 -- not an asteroid (will add it to exclusion list)
04:37:45.09 +69:31:52.6 -- not an asteroid (will add it to exclusion list)
05:42:30.68 +66:40:53.4 -- not an asteroid (will add it to exclusion list)
04:57:56.45 +70:12:50.7 -- not an asteroid (will add it to exclusion list)
05:12:57.41 +67:27:58.1 -- not an asteroid (will add it to exclusion list)
05:09:28.68 +68:58:24.5 -- not an asteroid (will add it to exclusion list)
04:52:10.93 +69:04:38.8 -- not an asteroid (will add it to exclusion list)
04:41:07.85 +69:52:14.2 -- not an asteroid (will add it to exclusion list)
04:17:52.79 +74:21:04.3 -- not an asteroid (will add it to exclusion list)
04:12:01.38 +72:33:10.6 -- not an asteroid (will add it to exclusion list)
04:33:00.02 +69:49:58.2 -- not an asteroid (will add it to exclusion list)
05:20:19.20 +66:54:36.3 -- not an asteroid (will add it to exclusion list)
04:55:08.75 +72:15:43.3 -- not an asteroid (will add it to exclusion list)
04:24:08.14 +70:35:51.0 -- not an asteroid (will add it to exclusion list)
05:21:10.60 +68:13:26.2 -- not an asteroid (will add it to exclusion list)
05:59:39.72 +66:33:45.1 -- not an asteroid (will add it to exclusion list)
04:34:38.43 +66:07:05.0 -- not an asteroid (will add it to exclusion list)
03:28:51.76 +73:05:52.8 -- not an asteroid (will add it to exclusion list)
04:13:42.88 +68:01:18.8 -- not an asteroid (will add it to exclusion list)
04:57:12.56 +65:29:17.0 -- not an asteroid (will add it to exclusion list)
05:48:53.85 +65:55:44.9 -- not an asteroid (will add it to exclusion list)
04:14:28.53 +66:30:56.2 -- not an asteroid (will add it to exclusion list)
05:25:14.34 +68:40:28.5 -- not an asteroid (will add it to exclusion list)
05:37:14.57 +70:27:32.7 -- not an asteroid (will add it to exclusion list)
05:50:48.26 +70:34:25.8 -- not an asteroid (will add it to exclusion list)
05:55:21.84 +65:57:48.7 -- not an asteroid (will add it to exclusion list)
03:45:57.33 +68:00:23.7 -- not an asteroid (will add it to exclusion list)
05:47:15.74 +63:52:31.3 -- not an asteroid (will add it to exclusion list)
05:29:05.20 +67:18:04.9 -- not an asteroid (will add it to exclusion list)
04:51:12.64 +68:13:48.0 -- not an asteroid (will add it to exclusion list)
05:57:01.15 +66:43:18.2 -- not an asteroid (will add it to exclusion list)
04:51:11.37 +68:13:32.8 -- not an asteroid (will add it to exclusion list)
04:42:00.42 +69:05:12.2 -- not an asteroid (will add it to exclusion list)
04:50:07.65 +67:38:39.4 -- not an asteroid (will add it to exclusion list)
04:45:32.04 +75:04:38.3 -- not an asteroid (will add it to exclusion list)
04:18:00.36 +71:14:00.4 -- not an asteroid (will add it to exclusion list)
05:25:17.07 +70:15:54.2 -- not an asteroid (will add it to exclusion list)
05:58:24.12 +68:08:34.9 -- not an asteroid (will add it to exclusion list)
05:31:25.46 +71:29:08.7 -- not an asteroid (will add it to exclusion list)
05:37:03.89 +74:14:30.2 -- not an asteroid (will add it to exclusion list)
05:25:27.56 +70:14:50.0 -- not an asteroid (will add it to exclusion list)
05:49:30.84 +65:53:52.6 -- not an asteroid (will add it to exclusion list)
05:50:01.72 +68:05:45.7 -- not an asteroid (will add it to exclusion list)
05:55:21.25 +68:02:16.3 -- not an asteroid (will add it to exclusion list)
05:16:19.61 +73:33:58.6 -- not an asteroid (will add it to exclusion list)
05:03:24.56 +68:22:02.2 -- not an asteroid (will add it to exclusion list)
05:15:08.71 +66:13:46.9 -- not an asteroid (will add it to exclusion list)
04:10:07.33 +68:21:09.6 -- not an asteroid (will add it to exclusion list)
05:29:51.44 +64:05:50.8 -- not an asteroid (will add it to exclusion list)
03:29:06.52 +72:34:22.7 -- not an asteroid (will add it to exclusion list)
04:27:17.52 +71:47:20.3 -- not an asteroid (will add it to exclusion list)
05:20:50.62 +66:51:55.2 -- not an asteroid (will add it to exclusion list)
04:50:07.29 +70:08:05.5 -- not an asteroid (will add it to exclusion list)
03:57:22.41 +71:25:04.5 -- not an asteroid (will add it to exclusion list)
04:54:12.65 +66:30:04.1 -- not an asteroid (will add it to exclusion list)
04:26:59.25 +67:44:49.8 -- not an asteroid (will add it to exclusion list)
05:43:11.16 +64:40:38.6 -- not an asteroid (will add it to exclusion list)
04:51:09.10 +68:10:39.5 -- not an asteroid (will add it to exclusion list)
04:24:04.98 +68:14:45.8 -- not an asteroid (will add it to exclusion list)
06:15:28.90 +71:02:58.6 -- not an asteroid (will add it to exclusion list)
04:24:03.71 +66:29:44.6 -- not an asteroid (will add it to exclusion list)
03:34:58.15 +71:38:57.5 -- not an asteroid (will add it to exclusion list)
06:03:16.16 +67:46:27.8 -- not an asteroid (will add it to exclusion list)
03:37:04.95 +69:37:38.9 -- not an asteroid (will add it to exclusion list)
04:39:51.44 +74:51:08.9 -- not an asteroid (will add it to exclusion list)
04:56:00.47 +72:50:48.4 -- not an asteroid (will add it to exclusion list)
04:48:44.31 +66:46:18.3 -- not an asteroid (will add it to exclusion list)
05:02:22.93 +65:05:21.9 -- not an asteroid (will add it to exclusion list)
05:13:15.58 +66:08:29.9 -- not an asteroid (will add it to exclusion list)
04:55:08.26 +66:57:32.4 -- not an asteroid (will add it to exclusion list)
06:22:42.85 +70:21:08.4 -- not an asteroid (will add it to exclusion list)
04:30:26.64 +69:08:36.1 -- not an asteroid (will add it to exclusion list)
05:32:49.67 +63:53:44.8 -- not an asteroid (will add it to exclusion list)
04:16:53.31 +69:09:51.9 -- not an asteroid (will add it to exclusion list)
04:45:00.00 +75:04:04.7 -- not an asteroid (will add it to exclusion list)
04:59:20.89 +74:13:58.3 -- not an asteroid (will add it to exclusion list)
05:27:12.08 +70:25:51.6 -- not an asteroid (will add it to exclusion list)
05:48:53.59 +67:06:07.5 -- not an asteroid (will add it to exclusion list)
05:15:06.43 +70:35:19.8 -- not an asteroid (will add it to exclusion list)
04:57:27.41 +68:33:28.0 -- not an asteroid (will add it to exclusion list)
06:25:26.55 +72:22:32.8 -- not an asteroid (will add it to exclusion list)
04:38:23.18 +65:27:17.1 -- not an asteroid (will add it to exclusion list)
05:52:47.83 +67:39:12.3 -- not an asteroid (will add it to exclusion list)
06:17:27.94 +71:50:59.3 -- not an asteroid (will add it to exclusion list)
05:25:41.83 +64:43:56.3 -- not an asteroid (will add it to exclusion list)
04:33:42.86 +69:30:55.3 -- not an asteroid (will add it to exclusion list)
05:44:30.23 +71:55:32.0 -- not an asteroid (will add it to exclusion list)
05:00:30.01 +70:04:35.1 -- not an asteroid (will add it to exclusion list)
06:23:58.93 +71:53:36.1 -- not an asteroid (will add it to exclusion list)
04:49:59.54 +70:21:41.5 -- not an asteroid (will add it to exclusion list)
05:22:57.96 +71:37:39.1 -- not an asteroid (will add it to exclusion list)
05:01:19.00 +71:44:34.6 -- not an asteroid (will add it to exclusion list)
06:23:30.24 +71:26:15.5 -- not an asteroid (will add it to exclusion list)
05:00:06.41 +74:34:47.1 -- not an asteroid (will add it to exclusion list)
03:59:25.51 +73:46:14.7 -- not an asteroid (will add it to exclusion list)
06:01:33.33 +68:08:08.1 -- not an asteroid (will add it to exclusion list)
05:54:19.71 +70:17:04.7 -- not an asteroid (will add it to exclusion list)
04:45:07.48 +74:15:01.9 -- not an asteroid (will add it to exclusion list)
05:20:14.92 +64:10:29.6 -- not an asteroid (will add it to exclusion list)
04:37:39.68 +68:10:37.6 -- not an asteroid (will add it to exclusion list)
04:47:24.76 +69:28:47.6 -- not an asteroid (will add it to exclusion list)
05:52:35.93 +67:07:30.8 -- not an asteroid (will add it to exclusion list)
06:31:24.90 +72:15:28.1 -- not an asteroid (will add it to exclusion list)
05:57:56.91 +73:38:45.0 -- not an asteroid (will add it to exclusion list)
05:50:09.91 +73:35:27.0 -- not an asteroid (will add it to exclusion list)
05:13:17.24 +70:20:12.0 -- not an asteroid (will add it to exclusion list)
05:31:33.34 +74:01:54.2 -- not an asteroid (will add it to exclusion list)
06:33:31.17 +71:47:37.8 -- not an asteroid (will add it to exclusion list)
04:12:00.38 +69:32:15.5 -- not an asteroid (will add it to exclusion list)
06:12:17.48 +70:34:57.0 -- not an asteroid (will add it to exclusion list)
05:44:33.84 +63:52:14.3 -- not an asteroid (will add it to exclusion list)
05:47:10.04 +66:16:05.9 -- not an asteroid (will add it to exclusion list)
04:39:36.65 +67:55:23.6 -- not an asteroid (will add it to exclusion list)
05:46:53.64 +69:24:30.3 -- not an asteroid (will add it to exclusion list)
05:34:28.21 +67:10:34.7 -- not an asteroid (will add it to exclusion list)
04:46:30.23 +70:37:03.2 -- not an asteroid (will add it to exclusion list)
06:03:10.68 +72:25:25.2 -- not an asteroid (will add it to exclusion list)
04:59:33.29 +74:03:12.1 -- not an asteroid (will add it to exclusion list)
03:55:44.87 +71:26:46.8 -- not an asteroid (will add it to exclusion list)
04:55:44.34 +74:31:21.0 -- not an asteroid (will add it to exclusion list)
05:28:51.13 +69:13:48.5 -- not an asteroid (will add it to exclusion list)
04:25:19.83 +70:27:54.6 -- not an asteroid (will add it to exclusion list)
05:28:29.50 +70:27:41.7 -- not an asteroid (will add it to exclusion list)
04:36:45.86 +72:15:20.8 -- not an asteroid (will add it to exclusion list)
05:04:12.63 +70:10:54.8 -- not an asteroid (will add it to exclusion list)
05:02:06.77 +73:08:34.6 -- not an asteroid (will add it to exclusion list)
05:00:58.15 +64:59:07.5 -- not an asteroid (will add it to exclusion list)
04:24:09.81 +67:08:23.9 -- not an asteroid (will add it to exclusion list)
04:55:40.07 +69:53:38.1 -- not an asteroid (will add it to exclusion list)
03:55:51.64 +66:08:49.5 -- not an asteroid (will add it to exclusion list)
04:51:56.19 +69:41:16.1 -- not an asteroid (will add it to exclusion list)
05:06:15.77 +64:55:52.5 -- not an asteroid (will add it to exclusion list)
04:41:06.02 +70:59:16.6 -- not an asteroid (will add it to exclusion list)
04:17:21.77 +72:57:07.1 -- not an asteroid (will add it to exclusion list)
05:30:42.74 +64:21:05.7 -- not an asteroid (will add it to exclusion list)
04:05:37.89 +66:19:58.3 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
03:28:51.76 +73:05:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:29:06.52 +72:34:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:58.15 +71:38:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:04.95 +69:37:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:25.91 +72:39:20.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:57.33 +68:00:23.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:55:44.87 +71:26:46.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:55:51.64 +66:08:49.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:57:22.41 +71:25:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:59:25.51 +73:46:14.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:37.89 +66:19:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:10:07.33 +68:21:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:12:00.38 +69:32:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:12:01.38 +72:33:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:13:42.88 +68:01:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:14:28.53 +66:30:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:16:53.31 +69:09:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:17:21.77 +72:57:07.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:17:52.79 +74:21:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:18:00.36 +71:14:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:03.71 +66:29:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:04.98 +68:14:45.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:08.14 +70:35:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:09.81 +67:08:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:19.83 +70:27:54.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:26:59.25 +67:44:49.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:27:17.52 +71:47:20.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:30:26.64 +69:08:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:00.02 +69:49:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:42.86 +69:30:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:34:38.43 +66:07:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:45.86 +72:15:20.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:39.68 +68:10:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:45.09 +69:31:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:38:23.18 +65:27:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:39:36.65 +67:55:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:39:51.44 +74:51:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:41:06.02 +70:59:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:41:07.85 +69:52:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:42:00.42 +69:05:12.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:45:00.00 +75:04:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:45:07.48 +74:15:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:45:32.04 +75:04:38.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:46:30.23 +70:37:03.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:47:24.76 +69:28:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:48:44.31 +66:46:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:49:59.54 +70:21:41.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:50:00.86 +68:10:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:50:07.29 +70:08:05.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:50:07.65 +67:38:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:51:09.10 +68:10:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:51:11.37 +68:13:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:51:12.64 +68:13:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:51:56.19 +69:41:16.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:52:10.93 +69:04:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:12.65 +66:30:04.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:08.26 +66:57:32.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:08.75 +72:15:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:40.07 +69:53:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:44.34 +74:31:21.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:00.47 +72:50:48.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:12.56 +65:29:17.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:27.41 +68:33:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:56.45 +70:12:50.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:20.89 +74:13:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:33.29 +74:03:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:06.41 +74:34:47.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:30.01 +70:04:35.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:58.15 +64:59:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:19.00 +71:44:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:06.77 +73:08:34.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:22.93 +65:05:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:24.56 +68:22:02.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:12.63 +70:10:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:15.77 +64:55:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:09:28.68 +68:58:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:12:57.41 +67:27:58.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:13:15.58 +66:08:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:13:17.24 +70:20:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:06.43 +70:35:19.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:08.71 +66:13:46.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:19.61 +73:33:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:59.75 +64:31:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:14.92 +64:10:29.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:19.20 +66:54:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:50.62 +66:51:55.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:10.60 +68:13:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:57.96 +71:37:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:14.34 +68:40:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:17.07 +70:15:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:27.56 +70:14:50.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:41.83 +64:43:56.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:12.08 +70:25:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:29.50 +70:27:41.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:51.13 +69:13:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:05.20 +67:18:04.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:51.44 +64:05:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:30:42.74 +64:21:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:25.46 +71:29:08.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:33.34 +74:01:54.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:49.67 +63:53:44.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:28.21 +67:10:34.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:03.89 +74:14:30.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:37:14.57 +70:27:32.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:30.68 +66:40:53.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:43:11.16 +64:40:38.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:30.23 +71:55:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:33.84 +63:52:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:53.64 +69:24:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:10.04 +66:16:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:15.74 +63:52:31.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:53.59 +67:06:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:53.85 +65:55:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:49:30.84 +65:53:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:01.72 +68:05:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:09.91 +73:35:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:48.26 +70:34:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:35.93 +67:07:30.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:47.83 +67:39:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:19.71 +70:17:04.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:21.25 +68:02:16.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:21.84 +65:57:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:01.15 +66:43:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:57:56.91 +73:38:45.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:24.12 +68:08:34.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:39.72 +66:33:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:33.33 +68:08:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:10.68 +72:25:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:16.16 +67:46:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:12:17.48 +70:34:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:15:28.90 +71:02:58.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:17:27.94 +71:50:59.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:22:42.85 +70:21:08.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:30.24 +71:26:15.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:58.93 +71:53:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:26.55 +72:22:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:31:24.90 +72:15:28.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:33:31.17 +71:47:37.8 -- 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)
03:28:51.76 +73:05:52.8 -- not a known variable star
03:29:06.52 +72:34:22.7 -- not a known variable star
03:34:58.15 +71:38:57.5 -- a known variable star
03:37:04.95 +69:37:38.9 -- not a known variable star
03:41:25.91 +72:39:20.4 -- not a known variable star
03:45:57.33 +68:00:23.7 -- not a known variable star
03:55:44.87 +71:26:46.8 -- not a known variable star
03:55:51.64 +66:08:49.5 -- not a known variable star
03:57:22.41 +71:25:04.5 -- not a known variable star
03:59:25.51 +73:46:14.7 -- not a known variable star
04:05:37.89 +66:19:58.3 -- a known variable star
04:10:07.33 +68:21:09.6 -- not a known variable star
04:12:00.38 +69:32:15.5 -- not a known variable star
04:12:01.38 +72:33:10.6 -- not a known variable star
04:13:42.88 +68:01:18.8 -- not a known variable star
04:14:28.53 +66:30:56.2 -- not a known variable star
04:16:53.31 +69:09:51.9 -- not a known variable star
04:17:21.77 +72:57:07.1 -- not a known variable star
04:17:52.79 +74:21:04.3 -- not a known variable star
04:18:00.36 +71:14:00.4 -- a known variable star
04:24:03.71 +66:29:44.6 -- not a known variable star
04:24:04.98 +68:14:45.8 -- not a known variable star
04:24:08.14 +70:35:51.0 -- not a known variable star
04:24:09.81 +67:08:23.9 -- not a known variable star
04:25:19.83 +70:27:54.6 -- not a known variable star
04:26:59.25 +67:44:49.8 -- a known variable star
04:27:17.52 +71:47:20.3 -- not a known variable star
04:30:26.64 +69:08:36.1 -- not a known variable star
04:33:00.02 +69:49:58.2 -- not a known variable star
04:33:42.86 +69:30:55.3 -- not a known variable star
04:34:38.43 +66:07:05.0 -- not a known variable star
04:36:45.86 +72:15:20.8 -- not a known variable star
04:37:39.68 +68:10:37.6 -- not a known variable star
04:37:45.09 +69:31:52.6 -- a known variable star
04:38:23.18 +65:27:17.1 -- not a known variable star
04:39:36.65 +67:55:23.6 -- not a known variable star
04:39:51.44 +74:51:08.9 -- not a known variable star
04:41:06.02 +70:59:16.6 -- not a known variable star
04:41:07.85 +69:52:14.2 -- not a known variable star
04:42:00.42 +69:05:12.2 -- not a known variable star
04:45:00.00 +75:04:04.7 -- not a known variable star
04:45:07.48 +74:15:01.9 -- not a known variable star
04:45:32.04 +75:04:38.3 -- not a known variable star
04:46:30.23 +70:37:03.2 -- not a known variable star
04:47:24.76 +69:28:47.6 -- not a known variable star
04:48:44.31 +66:46:18.3 -- not a known variable star
04:49:59.54 +70:21:41.5 -- not a known variable star
04:50:00.86 +68:10:46.4 -- not a known variable star
04:50:07.29 +70:08:05.5 -- not a known variable star
04:50:07.65 +67:38:39.4 -- not a known variable star
04:51:09.10 +68:10:39.5 -- not a known variable star
04:51:11.37 +68:13:32.8 -- not a known variable star
04:51:12.64 +68:13:48.0 -- not a known variable star
04:51:56.19 +69:41:16.1 -- not a known variable star
04:52:10.93 +69:04:38.8 -- not a known variable star
04:54:12.65 +66:30:04.1 -- not a known variable star
04:55:08.26 +66:57:32.4 -- not a known variable star
04:55:08.75 +72:15:43.3 -- not a known variable star
04:55:40.07 +69:53:38.1 -- not a known variable star
04:55:44.34 +74:31:21.0 -- not a known variable star
04:56:00.47 +72:50:48.4 -- not a known variable star
04:57:12.56 +65:29:17.0 -- not a known variable star
04:57:27.41 +68:33:28.0 -- not a known variable star
04:57:56.45 +70:12:50.7 -- not a known variable star
04:59:20.89 +74:13:58.3 -- not a known variable star
04:59:33.29 +74:03:12.1 -- not a known variable star
05:00:06.41 +74:34:47.1 -- not a known variable star
05:00:30.01 +70:04:35.1 -- not a known variable star
05:00:58.15 +64:59:07.5 -- not a known variable star
05:01:19.00 +71:44:34.6 -- not a known variable star
05:02:06.77 +73:08:34.6 -- not a known variable star
05:02:22.93 +65:05:21.9 -- not a known variable star
05:03:24.56 +68:22:02.2 -- not a known variable star
05:04:12.63 +70:10:54.8 -- not a known variable star
05:06:15.77 +64:55:52.5 -- not a known variable star
05:09:28.68 +68:58:24.5 -- not a known variable star
05:12:57.41 +67:27:58.1 -- not a known variable star
05:13:15.58 +66:08:29.9 -- not a known variable star
05:13:17.24 +70:20:12.0 -- not a known variable star
05:15:06.43 +70:35:19.8 -- not a known variable star
05:15:08.71 +66:13:46.9 -- not a known variable star
05:16:19.61 +73:33:58.6 -- not a known variable star
05:18:59.75 +64:31:42.7 -- not a known variable star
05:20:14.92 +64:10:29.6 -- not a known variable star
05:20:19.20 +66:54:36.3 -- not a known variable star
05:20:50.62 +66:51:55.2 -- not a known variable star
05:21:10.60 +68:13:26.2 -- not a known variable star
05:22:57.96 +71:37:39.1 -- not a known variable star
05:25:14.34 +68:40:28.5 -- not a known variable star
05:25:17.07 +70:15:54.2 -- not a known variable star
05:25:27.56 +70:14:50.0 -- not a known variable star
05:25:41.83 +64:43:56.3 -- not a known variable star
05:27:12.08 +70:25:51.6 -- not a known variable star
05:28:29.50 +70:27:41.7 -- not a known variable star
05:28:51.13 +69:13:48.5 -- not a known variable star
05:29:05.20 +67:18:04.9 -- not a known variable star
05:29:51.44 +64:05:50.8 -- not a known variable star
05:30:42.74 +64:21:05.7 -- not a known variable star
05:31:25.46 +71:29:08.7 -- not a known variable star
05:31:33.34 +74:01:54.2 -- not a known variable star
05:32:49.67 +63:53:44.8 -- not a known variable star
05:34:28.21 +67:10:34.7 -- a known variable star
05:37:03.89 +74:14:30.2 -- not a known variable star
05:37:14.57 +70:27:32.7 -- not a known variable star
05:42:30.68 +66:40:53.4 -- not a known variable star
05:43:11.16 +64:40:38.6 -- not a known variable star
05:44:30.23 +71:55:32.0 -- not a known variable star
05:44:33.84 +63:52:14.3 -- not a known variable star
05:46:53.64 +69:24:30.3 -- not a known variable star
05:47:10.04 +66:16:05.9 -- not a known variable star
05:47:15.74 +63:52:31.3 -- not a known variable star
05:48:53.59 +67:06:07.5 -- not a known variable star
05:48:53.85 +65:55:44.9 -- not a known variable star
05:49:30.84 +65:53:52.6 -- not a known variable star
05:50:01.72 +68:05:45.7 -- not a known variable star
05:50:09.91 +73:35:27.0 -- not a known variable star
05:50:48.26 +70:34:25.8 -- not a known variable star
05:52:35.93 +67:07:30.8 -- not a known variable star
05:52:47.83 +67:39:12.3 -- not a known variable star
05:54:19.71 +70:17:04.7 -- not a known variable star
05:55:21.25 +68:02:16.3 -- not a known variable star
05:55:21.84 +65:57:48.7 -- not a known variable star
05:57:01.15 +66:43:18.2 -- not a known variable star
05:57:56.91 +73:38:45.0 -- not a known variable star
05:58:24.12 +68:08:34.9 -- not a known variable star
05:59:39.72 +66:33:45.1 -- not a known variable star
06:01:33.33 +68:08:08.1 -- not a known variable star
06:03:10.68 +72:25:25.2 -- not a known variable star
06:03:16.16 +67:46:27.8 -- not a known variable star
06:12:17.48 +70:34:57.0 -- not a known variable star
06:15:28.90 +71:02:58.6 -- not a known variable star
06:17:27.94 +71:50:59.3 -- not a known variable star
06:22:42.85 +70:21:08.4 -- not a known variable star
06:23:30.24 +71:26:15.5 -- not a known variable star
06:23:58.93 +71:53:36.1 -- not a known variable star
06:25:26.55 +72:22:32.8 -- not a known variable star
06:31:24.90 +72:15:28.1 -- not a known variable star
06:33:31.17 +71:47:37.8 -- not a known variable star
Found 132 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
138 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 138 (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
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461121.78155735 -observatory 500
22:38:32.43 -07:53:48.3 Mercury (0.9mag)
01:12:24.81 +06:47:30.5 Venus (-3.9mag)
23:06:54.36 -06:50:49.2 Mars (1.2mag)
07:04:57.01 +22:57:47.0 Jupiter (-2.3mag)
00:17:56.14 -00:22:23.1 Saturn (0.9mag)
03:43:07.89 +19:32:31.9 Uranus (5.8mag)
00:07:28.10 -00:36:53.3 Neptune (7.8mag)
20:32:07.13 -22:53:37.6 Pluto (14.5mag)
02:40:56.88 +20:39:07.8 Moon (-9.1mag)
-rw-r--r-- 1 apache apache 361 Mar 22 01:49 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461121.78155735:
07:04:56.16 +22:57:51.4 Io (5.6mag)
07:05:03.29 +22:57:37.6 Europa (5.7mag)
07:04:41.38 +22:58:21.9 Ganymede (5.2mag)
07:04:19.18 +22:58:57.2 Callisto (6.4mag)
07:08:57.98 +22:58:39.0 Himalia (15.2mag)
07:04:52.31 +22:57:56.0 Thebe (16.1mag)
07:08:34.43 +23:22:29.5 Elara (17.2mag)
07:02:10.02 +23:50:47.2 Pasiphae (17.2mag)
07:13:43.41 +22:52:28.4 Carme (18.3mag)
00:17:55.08 -00:22:26.0 Titan (8.8mag)
00:17:59.87 -00:22:12.8 Rhea (10.1mag)
00:18:24.67 -00:20:16.9 Iapetus (11.5mag)
00:18:11.29 -00:22:23.5 Hyperion (14.8mag)
00:19:49.60 -00:11:13.2 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 22 01:49 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461121.78155735:
13:00:28.77 +07:29:03.0 JWST
18:25:36.13 +28:36:59.4 Chandra
17:24:39.08 -39:11:07.8 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 22 01:49 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461121.78155735 -observatory 500
-rw-r--r-- 1 apache apache 0 Mar 22 01:49 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
11:44:44.19 -62:10:45.50 ASASSN-26bq 2026-03-15.03 15.31
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 -0.22
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.41 -74:35:46.80 AT2026ahr 2026-01-20.09 16.98
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:25.13 +04:00:01.40 SN 2026kc 2026-01-18.24 16.4
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
-rw-r--r-- 1 apache apache 5.7K Mar 22 01:49 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 22 01:49 tocp_transients_list.txt
