Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.8949,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.3949 11.05CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:28:27.64 -26:56:45.7 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
UY Sco,2461098.8949,11.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
UY Sco 20260227.3949 11.22CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:14:40.30 -21:42:06.7 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CI Sco,2461098.8949,11.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CI Sco 20260227.3949 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:42:01.42 -29:45:07.6 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SSS_J162642.0-295716,2461098.8949,12.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SSS_J162642.0-295716 20260227.3949 12.13CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:26:41.99 -29:57:18.5 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461098.8949,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260227.3949 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 15:51:36.45 -23:53:07.5 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
VARIABLE_NAME,2461098.8949,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
VARIABLE_NAME 20260227.3949 13.10CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:39:39.24 -22:22:22.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
UZ Sco,2461098.8949,11.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
UZ Sco 20260227.3949 11.38CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:15:40.24 -25:01:02.2 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SSS_J160319.9-233220,2461098.8949,12.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SSS_J160319.9-233220 20260227.3949 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:03:19.75 -23:32:21.7 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GL Sco,2461098.8949,10.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GL Sco 20260227.3949 10.32CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:06:49.11 -22:38:41.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J160733-2941.3,2461098.8949,10.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J160733-2941.3 20260227.3949 10.62CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:07:33.32 -29:41:17.4 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V1328 Sco,2461098.8949,12.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
V1328 Sco 20260227.3949 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:03:31.85 -28:12:07.9 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
GU Sco,2461098.8949,11.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
GU Sco 20260227.3949 11.62CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:50:23.72 -28:11:35.0 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
TZ Sco,2461098.8949,11.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
TZ Sco 20260227.3949 11.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:07:42.86 -23:18:55.7 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
RX Sco,2461098.8949,10.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
RX Sco 20260227.3949 10.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:11:57.29 -24:53:56.8 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J161520-2919.6,2461098.8949,12.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J161520-2919.6 20260227.3949 12.18CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:15:20.41 -29:19:29.8 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J162405-2815.2,2461098.8949,9.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J162405-2815.2 20260227.3949 9.76CV 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/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:24:05.29 -28:15:13.3 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ASAS J161722-2455.5,2461098.8949,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASAS J161722-2455.5 20260227.3949 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-18_06-09-13_20.00sec_-14.90C_LIGHT_0016.fits /data_ssd/NMW-TexasTech/reference_imgs/Sco-02-Q2b1x1_2026-01-21_05-57-36_20.00sec_-15.00C_LIGHT_0588.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-03_20.00sec_-14.90C_LIGHT_0184.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-01_CI_Sco-02-Q2b1x1_065205_TTUQ2b1x1_8145_Ja5cPDkm/Sco-02-Q2b1x1_2026-02-27_03-28-53_20.00sec_-15.00C_LIGHT_0185.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 16:17:22.04 -24:55:32.0 ;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_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-53_20_00sec_-15_00C_LIGHT_0185_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Sco-02-Q2b1x1_2026-01-18_06-09-13_20_00sec_-14_90C_LIGHT_0016_fits__*pix.png resample_wcs_Sco-02-Q2b1x1_2026-02-27_03-28-03_20_00sec_-14_90C_LIGHT_0184_fits__*pix.png animation_v2.gif