This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz
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
Gaia DR3 498952020134255744,2461083.7942,13.76,0.05,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
Gaia DR3 498952020134255744 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:25:42.43 +72:10:43.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.53 05:03:00.83 +71:37:27.5
140.06853 17.75194 galactic Cam Second-epoch detections are separated by 1.9" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:00.83 +71:37:27.5 (user input) | T | P | (position from user input) J-Ks=0.436+/-0.050 (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,2461083.7942,13.53,0.05,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 20260212.2942 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:00.83 +71:37:27.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.81 05:48:21.87 +64:32:09.8
148.70844 17.92096 galactic Cam Second-epoch detections are separated by 3.4" and 4.6 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 | Large-amplitude variable Gaia DR2 287785073943782528 | 05:48:21.87 +64:32:09.8 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.462+/-0.044 (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
Large-amplitude variable Gaia DR2 287785073943782528,2461083.7942,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 287785073943782528 20260212.2942 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:21.87 +64:32:09.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.63 05:03:11.35 +69:43:42.8
141.72371 16.70557 galactic Cam Second-epoch detections are separated by 1.6" and 5.6 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 | target | 05:03:11.35 +69:43:42.8 (user input) | T | P | (position from user input) J-Ks=0.409+/-0.043 (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,2461083.7942,13.63,0.05,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 20260212.2942 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:11.35 +69:43:42.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.66,0.05,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 20260212.2942 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:18.16 +72:39:59.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.60 04:20:25.52 +74:02:55.8
136.04940 16.77877 galactic Cam Second-epoch detections are separated by 2.4" and 5.5 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 | target | 04:20:25.52 +74:02:55.8 (user input) | T | P | (position from user input) J-Ks=0.424+/-0.045 (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,2461083.7942,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:20:25.52 +74:02:55.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.46 04:33:03.65 +69:49:45.6
139.99707 14.70139 galactic Cam Second-epoch detections are separated by 0.6" and 5.6 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 | target | 04:33:03.65 +69:49:45.6 (user input) | T | P | (position from user input) J-Ks=0.473+/-0.038 (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,2461083.7942,13.46,0.05,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 20260212.2942 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:33:03.65 +69:49:45.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.42,0.05,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 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:06:37.63 +68:36:19.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.57 05:25:12.41 +66:12:18.6
145.98038 16.57585 galactic Cam Second-epoch detections are separated by 0.8" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:25:12.41 +66:12:18.6 (user input) | T | P | (position from user input) J-Ks=0.516+/-0.038 (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,2461083.7942,13.57,0.05,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 20260212.2942 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:25:12.41 +66:12:18.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.53 04:56:22.40 +72:43:26.7
138.81331 17.95202 galactic Cam Second-epoch detections are separated by 1.1" and 5.5 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 J074.1278+72.7191 | 04:56:22.40 +72:43:26.7 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.787+/-0.030 (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
ATO J074.1278+72.7191,2461083.7942,13.53,0.05,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
ATO J074.1278+72.7191 20260212.2942 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:22.40 +72:43:26.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.29 04:55:22.27 +66:47:32.8
143.77461 14.41654 galactic Cam Second-epoch detections are separated by 2.4" and 5.4 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 | target | 04:55:22.27 +66:47:32.8 (user input) | T | P | (position from user input) J-Ks=0.521+/-0.040 (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,2461083.7942,13.29,0.05,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 20260212.2942 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:55:22.27 +66:47:32.8 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.34 05:59:14.60 +70:12:05.1
143.65332 21.15971 galactic Cam Second-epoch detections are separated by 1.3" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J089.7975+70.2039 | 05:59:14.60 +70:12:05.1 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.457+/-0.039 (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
ATO J089.7975+70.2039,2461083.7942,13.34,0.05,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
ATO J089.7975+70.2039 20260212.2942 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:14.60 +70:12:05.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.20 04:49:37.46 +69:17:39.2
141.36985 15.48840 galactic Cam Second-epoch detections are separated by 2.6" and 5.5 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 | target | 04:49:37.46 +69:17:39.2 (user input) | T | P | (position from user input) J-Ks=0.469+/-0.038 (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,2461083.7942,13.20,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.20CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:37.46 +69:17:39.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.10 04:28:13.58 +68:28:43.7
140.74783 13.48545 galactic Cam Second-epoch detections are separated by 2.1" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 496562678286799744 | 04:28:12.90 +68:29:03.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.392+/-0.044 (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
Gaia DR3 496562678286799744,2461083.7942,13.10,0.05,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
Gaia DR3 496562678286799744 20260212.2942 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:28:13.58 +68:28:43.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.02 05:15:55.15 +73:39:59.9
138.77788 19.64920 galactic Cam Second-epoch detections are separated by 0.9" and 5.4 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 | target | 05:15:55.15 +73:39:59.9 (user input) | T | P | (position from user input) J-Ks=0.726+/-0.027 (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,2461083.7942,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:55.15 +73:39:59.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.15 06:14:59.89 +70:38:32.0
143.68739 22.55055 galactic Cam Second-epoch detections are separated by 1.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:14:59.89 +70:38:32.0 (user input) | T | P | (position from user input) J-Ks=0.270+/-0.045 (F)
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,2461083.7942,13.15,0.05,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 20260212.2942 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:59.89 +70:38:32.0 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.15 05:01:49.26 +66:03:52.6
144.77392 14.51190 galactic Cam Second-epoch detections are separated by 1.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:01:49.26 +66:03:52.6 (user input) | T | P | (position from user input) J-Ks=0.480+/-0.037 (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,2461083.7942,13.15,0.05,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 20260212.2942 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:01:49.26 +66:03:52.6 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.16 05:34:40.32 +67:06:25.9
145.63366 17.83391 galactic Cam Second-epoch detections are separated by 3.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:34:40.32 +67:06:25.9 (user input) | T | P | (position from user input) J-Ks=0.620+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:40.32 +67:06:25.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 496074671221247232,2461083.7942,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 496074671221247232 20260212.2942 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:54:19.78 +68:57:49.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.87 05:02:53.80 +65:01:14.0
145.71953 13.99956 galactic Cam Second-epoch detections are separated by 0.5" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:02:53.80 +65:01:14.0 (user input) | T | P | (position from user input) J-Ks=0.431+/-0.034 (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,2461083.7942,12.87,0.05,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 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:02:53.80 +65:01:14.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,12.96,0.05,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 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:32:28.63 +67:14:24.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.74 04:02:19.72 +70:42:08.6
137.49273 13.44458 galactic Cam Second-epoch detections are separated by 1.1" and 5.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:02:19.72 +70:42:08.6 (user input) | T | P | (position from user input) J-Ks=0.757+/-0.029 (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,2461083.7942,12.74,0.05,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
target 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:02:19.72 +70:42:08.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 485930405145239808,2461083.7942,12.72,0.05,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
Gaia DR3 485930405145239808 20260212.2942 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:38:34.63 +70:25:44.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.77 05:13:00.11 +68:41:29.0
143.12803 16.86597 galactic Cam Second-epoch detections are separated by 0.4" 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 | target | 05:13:00.11 +68:41:29.0 (user input) | T | P | (position from user input) J-Ks=0.380+/-0.038 (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,2461083.7942,12.77,0.05,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 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:13:00.11 +68:41:29.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.44 03:24:31.89 +70:39:05.7
135.01891 11.46350 galactic Cas Second-epoch detections are separated by 1.0" 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 | Gaia DR3 543001204721358976 | 03:24:33.97 +70:38:48.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.493+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2942* 03 24 31.89 +70 39 05.7 12.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543001204721358976,2461083.7942,12.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543001204721358976 20260212.2942 12.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:24:31.89 +70:39:05.7 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.35 05:44:46.41 +64:00:07.9
149.02971 17.33516 galactic Cam Second-epoch detections are separated by 0.1" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:44:46.41 +64:00:07.9 (user input) | T | P | (position from user input) J-Ks=0.373+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,12.35,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 12.35CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:44:46.41 +64:00:07.9 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J052712.24+723426.3,2461083.7942,12.01,0.05,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
ASASSN-V J052712.24+723426.3 20260212.2942 12.01CV 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:27:07.63 +72:34:27.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 11.90 05:52:27.86 +70:32:03.8
143.09201 20.75935 galactic Cam Second-epoch detections are separated by 0.5" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:52:27.86 +70:32:03.8 (user input) | T | P | (position from user input) J-Ks=0.316+/-0.034 (F)
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,2461083.7942,11.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 11.90CV 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:52:27.86 +70:32:03.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 11.38 03:45:58.83 +68:00:22.9
138.16832 10.46143 galactic Cam Second-epoch detections are separated by 1.9" 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 | Gaia DR3 493476112928592512 | 03:45:59.00 +68:00:23.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.977+/-0.033 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 493476112928592512,2461083.7942,11.38,0.05,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
Gaia DR3 493476112928592512 20260212.2942 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:58.83 +68:00:22.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 11.66 04:42:14.62 +69:04:10.2
141.13418 14.83361 galactic Cam Second-epoch detections are separated by 0.3" and 5.6 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 | target | 04:42:14.62 +69:04:10.2 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.031 (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,2461083.7942,11.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 11.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:42:14.62 +69:04:10.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 11.99 04:57:37.94 +70:38:34.8
140.65848 16.83826 galactic Cam Second-epoch detections are separated by 0.5" and 5.5 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 | target | 04:57:37.94 +70:38:34.8 (user input) | T | P | (position from user input) J-Ks=0.643+/-0.033 (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,2461083.7942,11.99,0.05,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 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:57:37.94 +70:38:34.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.18 04:48:51.80 +74:27:59.9
136.99583 18.53286 galactic Cam Second-epoch detections are separated by 0.3" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 502054777524725504 | 04:48:48.71 +74:28:20.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.273+/-0.031 (F)
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 502054777524725504,2461083.7942,12.18,0.05,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
Gaia DR3 502054777524725504 20260212.2942 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:48:51.80 +74:27:59.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.26 05:32:38.74 +71:28:25.8
141.45790 19.69654 galactic Cam Second-epoch detections are separated by 0.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 498286407580396416 | 05:32:44.24 +71:28:48.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.634+/-0.034 (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
Gaia DR3 498286407580396416,2461083.7942,12.26,0.05,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
Gaia DR3 498286407580396416 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:32:38.74 +71:28:25.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.48 05:38:30.12 +74:15:31.5
138.98765 21.30511 galactic Cam Second-epoch detections are separated by 0.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 499744359997648256 | 05:38:26.91 +74:15:01.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.608+/-0.033 (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
Gaia DR3 499744359997648256,2461083.7942,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 499744359997648256 20260212.2942 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:38:30.12 +74:15:31.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.53 05:45:07.80 +70:54:04.3
142.47293 20.35302 galactic Cam Second-epoch detections are separated by 0.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 486153983962515840 | 05:45:13.11 +70:54:00.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.465+/-0.039 (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
Gaia DR3 486153983962515840,2461083.7942,12.53,0.05,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
Gaia DR3 486153983962515840 20260212.2942 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:45:07.80 +70:54:04.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.48 05:51:35.41 +68:00:53.7
145.52076 19.68237 galactic Cam Second-epoch detections are separated by 0.7" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:51:35.41 +68:00:53.7 (user input) | T | P | (position from user input) J-Ks=0.327+/-0.037 (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,2461083.7942,12.48,0.05,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 20260212.2942 12.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:35.41 +68:00:53.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.55 03:37:05.47 +69:37:35.6
136.51175 11.25018 galactic Cas Second-epoch detections are separated by 0.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:37:05.47 +69:37:35.6 (user input) | T | P | (position from user input) J-Ks=0.526+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2942* 03 37 05.47 +69 37 35.6 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
target,2461083.7942,12.55,0.05,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 20260212.2942 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:05.47 +69:37:35.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.63 05:17:15.82 +73:34:58.5
138.90525 19.68924 galactic Cam Second-epoch detections are separated by 1.0" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:17:15.82 +73:34:58.5 (user input) | T | P | (position from user input) J-Ks=0.272+/-0.031 (F)
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,2461083.7942,12.63,0.05,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
target 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:15.82 +73:34:58.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.78 05:48:53.23 +73:08:42.4
140.39797 21.52069 galactic Cam Second-epoch detections are separated by 1.1" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 498718068972360960 | 05:48:57.23 +73:09:03.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.357+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 498718068972360960,2461083.7942,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 498718068972360960 20260212.2942 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:53.23 +73:08:42.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.68 05:42:16.32 +68:55:14.9
144.26729 19.28878 galactic Cam Second-epoch detections are separated by 0.8" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 484811892582144896 | 05:42:13.98 +68:55:36.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.572+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 484811892582144896,2461083.7942,12.68,0.05,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
Gaia DR3 484811892582144896 20260212.2942 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:42:16.32 +68:55:14.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.78 04:03:46.01 +74:47:17.6
134.68113 16.49908 galactic Cam Second-epoch detections are separated by 2.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 549963797683423488 | 04:03:55.43 +74:47:30.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.391+/-0.037 (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
Gaia DR3 549963797683423488,2461083.7942,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 549963797683423488 20260212.2942 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:03:46.01 +74:47:17.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,12.72,0.05,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 20260212.2942 12.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:07.64 +66:28:21.7 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.68 04:41:23.25 +72:55:31.7
137.95252 17.18352 galactic Cam Second-epoch detections are separated by 1.4" 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 | target | 04:41:23.25 +72:55:31.7 (user input) | T | P | (position from user input) J-Ks=0.411+/-0.040 (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,2461083.7942,12.68,0.05,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 20260212.2942 12.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:41:23.25 +72:55:31.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 483292298793027456,2461083.7942,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 483292298793027456 20260212.2942 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:57.56 +67:08:31.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2942* 03 34 59.11 +71 38 54.0 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 543153422658023040,2461083.7942,12.89,0.05,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
Gaia DR3 543153422658023040 20260212.2942 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:34:59.11 +71:38:54.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.88 04:46:14.94 +66:27:36.0
143.47821 13.49664 galactic Cam Second-epoch detections are separated by 0.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 483234810651741952 | 04:46:12.01 +66:27:04.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.932+/-0.033 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 483234810651741952,2461083.7942,12.88,0.05,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
Gaia DR3 483234810651741952 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:46:14.94 +66:27:36.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.90 03:58:46.26 +73:22:06.9
135.42666 15.22697 galactic Cam Second-epoch detections are separated by 3.2" 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 | target | 03:58:46.26 +73:22:06.9 (user input) | T | P | (position from user input) J-Ks=0.657+/-0.029 (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,2461083.7942,12.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 12.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:58:46.26 +73:22:06.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 12.88 05:53:04.13 +64:13:56.7
149.22622 18.25029 galactic Cam Second-epoch detections are separated by 1.3" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 287049225785639808 | 05:53:04.68 +64:14:20.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.487+/-0.028 (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
Gaia DR3 287049225785639808,2461083.7942,12.88,0.05,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
Gaia DR3 287049225785639808 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:04.13 +64:13:56.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:29:18.98 +69:31:54.8 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.04 04:20:01.28 +68:13:24.2
140.40984 12.75780 galactic Cam Second-epoch detections are separated by 2.7" 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 | target | 04:20:01.28 +68:13:24.2 (user input) | T | P | (position from user input) J-Ks=0.467+/-0.046 (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,2461083.7942,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.04CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:20:01.28 +68:13:24.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.05 04:54:50.65 +66:57:16.2
143.60837 14.47153 galactic Cam Second-epoch detections are separated by 1.0" and 5.6 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 | target | 04:54:50.65 +66:57:16.2 (user input) | T | P | (position from user input) J-Ks=0.469+/-0.038 (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,2461083.7942,13.05,0.05,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 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:54:50.65 +66:57:16.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 287880976270002944,2461083.7942,13.12,0.05,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
Gaia DR3 287880976270002944 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:22.12 +64:43:30.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.15 05:02:57.10 +65:09:02.1
145.61355 14.07937 galactic Cam Second-epoch detections are separated by 1.6" and 5.5 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 | target | 05:02:57.10 +65:09:02.1 (user input) | T | P | (position from user input) J-Ks=0.348+/-0.041 (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,2461083.7942,13.15,0.05,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 20260212.2942 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:02:57.10 +65:09:02.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
ZTF J051555.95+703407.7,2461083.7942,12.98,0.05,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
ZTF J051555.95+703407.7 20260212.2942 12.98CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:57.20 +70:34:25.2 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.15 06:25:10.05 +70:16:23.9
144.33810 23.25756 galactic Cam Second-epoch detections are separated by 2.5" and 4.2 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 1107464880713500416 | 06:25:10.09 +70:16:50.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.355+/-0.038 (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
Gaia DR3 1107464880713500416,2461083.7942,13.15,0.05,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
Gaia DR3 1107464880713500416 20260212.2942 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:25:10.05 +70:16:23.9 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.10 05:26:37.67 +64:37:46.4
147.47469 15.90793 galactic Cam Second-epoch detections are separated by 0.9" and 5.6 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 479765477806636032 | 05:26:37.70 +64:37:18.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.702+/-0.035 (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
Gaia DR3 479765477806636032,2461083.7942,13.10,0.05,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
Gaia DR3 479765477806636032 20260212.2942 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/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:26:37.67 +64:37:46.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.15,0.05,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 20260212.2942 13.15CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:36:37.21 +74:18:46.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.03 05:54:33.59 +72:46:27.0
140.93687 21.76437 galactic Cam Second-epoch detections are separated by 1.4" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 498478268060538752 | 05:54:36.38 +72:46:02.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.536+/-0.033 (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
Gaia DR3 498478268060538752,2461083.7942,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 498478268060538752 20260212.2942 13.03CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:33.59 +72:46:27.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.17 05:01:18.34 +66:42:39.3
144.19774 14.84311 galactic Cam Second-epoch detections are separated by 0.9" and 5.6 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 482844587103106432 | 05:01:15.76 +66:43:03.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.744+/-0.035 (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
Gaia DR3 482844587103106432,2461083.7942,13.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 482844587103106432 20260212.2942 13.17CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:01:18.34 +66:42:39.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.25 03:35:57.74 +72:27:17.7
134.69643 13.45561 galactic Cas Second-epoch detections are separated by 0.8" 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 | target | 03:35:57.74 +72:27:17.7 (user input) | T | P | (position from user input) J-Ks=0.919+/-0.034 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2942* 03 35 57.74 +72 27 17.7 13.2 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.25,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.25CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:35:57.74 +72:27:17.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 496326425025087744,2461083.7942,13.23,0.05,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
Gaia DR3 496326425025087744 20260212.2942 13.23CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:47:41.50 +69:27:47.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.34 05:36:57.85 +65:42:05.7
147.04910 17.37769 galactic Cam Second-epoch detections are separated by 2.2" and 5.4 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 480103234034360576 | 05:37:03.54 +65:42:20.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.746+/-0.031 (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
Gaia DR3 480103234034360576,2461083.7942,13.34,0.05,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 480103234034360576 20260212.2942 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:36:57.85 +65:42:05.7 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.26,0.05,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 20260212.2942 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:19.03 +72:42:38.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.26 05:38:13.79 +68:50:54.9
144.16540 18.93035 galactic Cam Second-epoch detections are separated by 2.4" and 5.4 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 484802267556955520 | 05:38:18.81 +68:50:47.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.438+/-0.050 (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
Gaia DR3 484802267556955520,2461083.7942,13.26,0.05,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
Gaia DR3 484802267556955520 20260212.2942 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:38:13.79 +68:50:54.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.29 04:45:29.78 +74:16:14.4
137.01940 18.23396 galactic Cam Second-epoch detections are separated by 1.2" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:45:29.78 +74:16:14.4 (user input) | T | P | (position from user input) J-Ks=0.435+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.29,0.05,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 20260212.2942 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:45:29.78 +74:16:14.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 1113701345025390720,2461083.7942,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1113701345025390720 20260212.2942 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:28:02.54 +72:19:51.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.29 05:44:29.09 +70:20:34.0
142.98978 20.07116 galactic Cam Second-epoch detections are separated by 2.5" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 485889517056731520 | 05:44:35.80 +70:20:06.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.824+/-0.032 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 485889517056731520,2461083.7942,13.29,0.05,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
Gaia DR3 485889517056731520 20260212.2942 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:44:29.09 +70:20:34.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 495945341166905216,2461083.7942,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 495945341166905216 20260212.2942 13.27CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:40:44.25 +69:05:34.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.26 04:49:42.22 +75:05:48.9
136.49128 18.94759 galactic Cam Second-epoch detections are separated by 1.7" and 5.6 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 | ATO J072.4256+75.0970 | 04:49:42.22 +75:05:48.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.636+/-0.034 (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
ATO J072.4256+75.0970,2461083.7942,13.26,0.05,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
ATO J072.4256+75.0970 20260212.2942 13.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:42.22 +75:05:48.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:13.15 +67:07:08.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.40 04:30:44.57 +74:12:33.4
136.41278 17.41327 galactic Cam Second-epoch detections are separated by 1.9" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 501995713134593664 | 04:30:49.96 +74:13:05.6 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.754+/-0.031 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 501995713134593664,2461083.7942,13.40,0.05,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
Large-amplitude variable Gaia DR2 501995713134593664 20260212.2942 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:30:44.57 +74:12:33.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.29 04:54:16.84 +65:21:23.2
144.89135 13.46805 galactic Cam Second-epoch detections are separated by 1.5" 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 | target | 04:54:16.84 +65:21:23.2 (user input) | T | P | (position from user input) J-Ks=0.377+/-0.039 (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,2461083.7942,13.29,0.05,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 20260212.2942 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:54:16.84 +65:21:23.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.48 03:20:24.91 +70:25:30.5
134.85656 11.08472 galactic Cas Second-epoch detections are separated by 0.8" 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 | target | 03:20:24.91 +70:25:30.5 (user input) | T | P | (position from user input) J-Ks=0.530+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2942* 03 20 24.91 +70 25 30.5 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.48,0.05,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 20260212.2942 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:20:24.91 +70:25:30.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.43 04:41:44.13 +74:34:43.8
136.60025 18.22019 galactic Cam Second-epoch detections are separated by 2.6" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 502092229639747328 | 04:41:53.62 +74:34:34.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.324+/-0.053 (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
Gaia DR3 502092229639747328,2461083.7942,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 502092229639747328 20260212.2942 13.43CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:41:44.13 +74:34:43.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:14:38.82 +70:39:51.6 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 503562207967629952,2461083.7942,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 503562207967629952 20260212.2942 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:53:44.19 +74:47:25.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.38,0.05,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 20260212.2942 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:14:05.29 +70:19:07.5 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.40 05:11:19.59 +72:08:05.9
139.98397 18.57167 galactic Cam Second-epoch detections are separated by 1.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:11:19.59 +72:08:05.9 (user input) | T | P | (position from user input) J-Ks=0.313+/-0.046 (F)
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,2461083.7942,13.40,0.05,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 20260212.2942 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:11:19.59 +72:08:05.9 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WISE J053339.5+642307,2461083.7942,13.56,0.05,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
WISE J053339.5+642307 20260212.2942 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:33:39.65 +64:23:07.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.58 05:24:32.25 +69:38:25.8
142.82603 18.23318 galactic Cam Second-epoch detections are separated by 0.8" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:24:32.25 +69:38:25.8 (user input) | T | P | (position from user input) J-Ks=0.330+/-0.041 (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,2461083.7942,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:24:32.25 +69:38:25.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.34 03:20:56.37 +71:13:17.8
134.44601 11.77341 galactic Cas Second-epoch detections are separated by 3.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:20:56.37 +71:13:17.8 (user input) | T | P | (position from user input) J-Ks=0.839+/-0.035 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2942* 03 20 56.37 +71 13 17.8 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.34,0.05,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 20260212.2942 13.34CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:20:56.37 +71:13:17.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.53 05:50:23.86 +67:00:17.6
146.44665 19.16210 galactic Cam Second-epoch detections are separated by 1.8" 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 | target | 05:50:23.86 +67:00:17.6 (user input) | T | P | (position from user input) J-Ks=0.644+/-0.037 (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,2461083.7942,13.53,0.05,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 20260212.2942 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:50:23.86 +67:00:17.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.52 03:42:15.16 +71:59:39.0
135.37656 13.38442 galactic Cam Second-epoch detections are separated by 2.4" 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 | 03:42:15.16 +71:59:39.0 (user input) | T | P | (position from user input) J-Ks=0.700+/-0.035 (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,2461083.7942,13.52,0.05,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 20260212.2942 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:42:15.16 +71:59:39.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.48 04:24:34.43 +69:53:54.5
139.44213 14.20194 galactic Cam Second-epoch detections are separated by 0.3" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 496933870838722048 | 04:24:27.70 +69:53:26.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A 1956PMcCO..13a....B AG+69 197 J-Ks=0.524+/-0.037 (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
Gaia DR3 496933870838722048,2461083.7942,13.48,0.05,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
Gaia DR3 496933870838722048 20260212.2942 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:34.43 +69:53:54.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:32:13.20 +69:46:33.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.61 03:41:25.57 +68:24:22.9
137.57895 10.51462 galactic Cam Second-epoch detections are separated by 0.8" 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 | target | 03:41:25.57 +68:24:22.9 (user input) | T | P | (position from user input) J-Ks=0.416+/-0.038 (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,2461083.7942,13.61,0.05,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 20260212.2942 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:25.57 +68:24:22.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 479516575867094528,2461083.7942,13.38,0.05,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
Gaia DR3 479516575867094528 20260212.2942 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:08.88 +65:22:12.0 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.38 03:36:50.18 +72:50:03.8
134.51418 13.79748 galactic Cas Second-epoch detections are separated by 3.0" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:36:50.18 +72:50:03.8 (user input) | T | P | (position from user input) J-Ks=0.784+/-0.031 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2942* 03 36 50.18 +72 50 03.8 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.38,0.05,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 20260212.2942 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:36:50.18 +72:50:03.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2942* 03 25 13.90 +73 15 13.9 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544468782163850880,2461083.7942,13.50,0.05,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
Gaia DR3 544468782163850880 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:25:13.90 +73:15:13.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.41 06:07:10.79 +71:30:10.3
142.58645 22.22467 galactic Cam Second-epoch detections are separated by 2.0" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:07:10.79 +71:30:10.3 (user input) | T | P | (position from user input) J-Ks=0.432+/-0.037 (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,2461083.7942,13.41,0.05,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 20260212.2942 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:10.79 +71:30:10.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.54 05:36:48.01 +64:22:23.6
148.26628 16.73674 galactic Cam Second-epoch detections are separated by 1.2" and 5.5 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 | target | 05:36:48.01 +64:22:23.6 (user input) | T | P | (position from user input) J-Ks=0.368+/-0.050 (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,2461083.7942,13.54,0.05,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 20260212.2942 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:36:48.01 +64:22:23.6 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
V0560 Cam,2461083.7942,13.41,0.05,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
V0560 Cam 20260212.2942 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:10:05.98 +69:59:13.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.56 04:09:14.33 +70:14:49.4
138.24586 13.50972 galactic Cam Second-epoch detections are separated by 2.6" 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 | target | 04:09:14.33 +70:14:49.4 (user input) | T | P | (position from user input) J-Ks=0.742+/-0.029 (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,2461083.7942,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:09:14.33 +70:14:49.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.62 03:56:03.36 +69:57:43.5
137.59633 12.54108 galactic Cam Second-epoch detections are separated by 1.2" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:56:03.36 +69:57:43.5 (user input) | T | P | (position from user input) J-Ks=0.430+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.62,0.05,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 20260212.2942 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:03.36 +69:57:43.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.48 05:22:05.63 +66:32:17.4
145.51585 16.47660 galactic Cam Second-epoch detections are separated by 0.5" 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 | target | 05:22:05.63 +66:32:17.4 (user input) | T | P | (position from user input) J-Ks=0.470+/-0.047 (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,2461083.7942,13.48,0.05,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 20260212.2942 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:22:05.63 +66:32:17.4 ;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_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.47 03:37:19.76 +67:04:59.2
138.07692 9.22596 galactic Cam Second-epoch detections are separated by 0.6" 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 | target | 03:37:19.76 +67:04:59.2 (user input) | T | P | (position from user input) J-Ks=0.984+/-0.034 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:19.76 +67:04:59.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.59 03:53:39.59 +67:23:17.3
139.13978 10.44701 galactic Cam Second-epoch detections are separated by 2.5" 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 | target | 03:53:39.59 +67:23:17.3 (user input) | T | P | (position from user input) J-Ks=0.507+/-0.035 (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,2461083.7942,13.59,0.05,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 20260212.2942 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:39.59 +67:23:17.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.44 05:19:37.55 +70:19:20.9
141.98304 18.20915 galactic Cam Second-epoch detections are separated by 0.9" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:19:37.55 +70:19:20.9 (user input) | T | P | (position from user input) J-Ks=0.465+/-0.036 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:19:37.55 +70:19:20.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.65 05:18:23.35 +72:55:11.7
139.55803 19.42890 galactic Cam Second-epoch detections are separated by 1.9" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:18:23.35 +72:55:11.7 (user input) | T | P | (position from user input) J-Ks=0.445+/-0.049 (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,2461083.7942,13.65,0.05,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 20260212.2942 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:18:23.35 +72:55:11.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.58 05:11:29.94 +74:28:23.6
137.87636 19.79866 galactic Cam Second-epoch detections are separated by 1.1" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:11:29.94 +74:28:23.6 (user input) | T | P | (position from user input) J-Ks=0.357+/-0.046 (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,2461083.7942,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:11:29.94 +74:28:23.6 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.30 03:33:02.07 +68:48:58.5
136.70638 10.38448 galactic Cas Second-epoch detections are separated by 1.6" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:33:02.07 +68:48:58.5 (user input) | T | P | (position from user input) J-Ks=0.480+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2942* 03 33 02.07 +68 48 58.5 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.30CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:33:02.07 +68:48:58.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.61 05:45:03.32 +65:00:23.3
148.10161 17.81125 galactic Cam Second-epoch detections are separated by 1.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:45:03.32 +65:00:23.3 (user input) | T | P | (position from user input) J-Ks=0.470+/-0.042 (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,2461083.7942,13.61,0.05,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 20260212.2942 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:45:03.32 +65:00:23.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.62 03:25:02.01 +73:22:53.5
133.46906 13.73654 galactic Cas Second-epoch detections are separated by 5.0" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:25:02.01 +73:22:53.5 (user input) | T | P | (position from user input) J-Ks=0.770+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2942* 03 25 02.01 +73 22 53.5 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.62,0.05,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 20260212.2942 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:25:02.01 +73:22:53.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.69 05:06:40.14 +64:59:44.7
145.97556 14.31219 galactic Cam Second-epoch detections are separated by 1.7" 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 | target | 05:06:40.14 +64:59:44.7 (user input) | T | P | (position from user input) J-Ks=0.683+/-0.035 (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,2461083.7942,13.69,0.05,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 20260212.2942 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:06:40.14 +64:59:44.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.44 04:10:48.95 +74:38:56.2
135.12880 16.72506 galactic Cam Second-epoch detections are separated by 3.0" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:10:48.95 +74:38:56.2 (user input) | T | P | (position from user input) J-Ks=0.507+/-0.041 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:10:48.95 +74:38:56.2 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.50 03:43:52.01 +74:14:46.5
134.01756 15.21513 galactic Cam Second-epoch detections are separated by 1.4" 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 | target | 03:43:52.01 +74:14:46.5 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.053 (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,2461083.7942,13.50,0.05,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 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:52.01 +74:14:46.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.48 04:18:40.06 +75:11:20.7
135.09069 17.46746 galactic Cam Second-epoch detections are separated by 2.1" and 5.5 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 | Large-amplitude variable Gaia DR2 550316294237745536 | 04:18:40.06 +75:11:20.7 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.306+/-0.042 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 550316294237745536,2461083.7942,13.48,0.05,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
Large-amplitude variable Gaia DR2 550316294237745536 20260212.2942 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:18:40.06 +75:11:20.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.41,0.05,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 20260212.2942 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:31:19.79 +67:14:13.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.60 05:29:51.31 +72:20:59.5
140.52497 19.90589 galactic Cam Second-epoch detections are separated by 1.1" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:29:51.31 +72:20:59.5 (user input) | T | P | (position from user input) J-Ks=0.436+/-0.047 (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,2461083.7942,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:51.31 +72:20:59.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.50 04:21:07.90 +66:11:01.9
141.98800 11.41988 galactic Cam Second-epoch detections are separated by 1.7" 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 | target | 04:21:07.90 +66:11:01.9 (user input) | T | P | (position from user input) J-Ks=0.521+/-0.036 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.50,0.05,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 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:21:07.90 +66:11:01.9 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.56 05:13:28.28 +65:11:51.8
146.21326 15.01977 galactic Cam Second-epoch detections are separated by 2.1" and 5.6 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 | target | 05:13:28.28 +65:11:51.8 (user input) | T | P | (position from user input) J-Ks=0.414+/-0.037 (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,2461083.7942,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:13:28.28 +65:11:51.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 482088471000996736,2461083.7942,13.64,0.05,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 482088471000996736 20260212.2942 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:54:44.77 +65:04:13.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.49 03:55:47.22 +71:26:44.6
136.57589 13.64282 galactic Cam Second-epoch detections are separated by 1.4" 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 | target | 03:55:47.22 +71:26:44.6 (user input) | T | P | (position from user input) J-Ks=0.541+/-0.058 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.49,0.05,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 20260212.2942 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:55:47.22 +71:26:44.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.52 03:22:47.79 +73:32:35.9
133.23970 13.77991 galactic Cas Second-epoch detections are separated by 0.4" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:22:47.79 +73:32:35.9 (user input) | T | P | (position from user input) J-Ks=0.501+/-0.036 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2942* 03 22 47.79 +73 32 35.9 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.52,0.05,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 20260212.2942 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:22:47.79 +73:32:35.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.49,0.05,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 20260212.2942 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:52.72 +67:13:28.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.52 04:25:22.03 +65:57:39.5
142.45477 11.57765 galactic Cam Second-epoch detections are separated by 1.2" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:25:22.03 +65:57:39.5 (user input) | T | P | (position from user input) J-Ks=0.517+/-0.058 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.52,0.05,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 20260212.2942 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:22.03 +65:57:39.5 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.74 05:34:52.29 +63:51:44.1
148.62940 16.30756 galactic Cam Second-epoch detections are separated by 0.5" 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 | target | 05:34:52.29 +63:51:44.1 (user input) | T | P | (position from user input) J-Ks=0.487+/-0.042 (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,2461083.7942,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:52.29 +63:51:44.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.69 05:16:24.61 +64:47:32.3
146.74028 15.06167 galactic Cam Second-epoch detections are separated by 0.2" and 5.5 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 | target | 05:16:24.61 +64:47:32.3 (user input) | T | P | (position from user input) J-Ks=0.387+/-0.037 (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,2461083.7942,13.69,0.05,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 20260212.2942 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:16:24.61 +64:47:32.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.45 05:35:04.26 +72:27:17.1
140.61508 20.30496 galactic Cam Second-epoch detections are separated by 1.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:35:04.26 +72:27:17.1 (user input) | T | P | (position from user input) J-Ks=0.668+/-0.039 (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,2461083.7942,13.45,0.05,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 20260212.2942 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:35:04.26 +72:27:17.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.57 04:24:11.80 +67:34:12.8
141.17255 12.59305 galactic Cam Second-epoch detections are separated by 3.3" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:24:11.80 +67:34:12.8 (user input) | T | P | (position from user input) J-Ks=0.416+/-0.033 (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,2461083.7942,13.57,0.05,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 20260212.2942 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:11.80 +67:34:12.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.55 04:37:49.74 +72:49:37.5
137.86183 16.91748 galactic Cam Second-epoch detections are separated by 2.3" and 5.6 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 500874206976672384 | 04:37:55.32 +72:49:56.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.418+/-0.044 (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
Gaia DR3 500874206976672384,2461083.7942,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 500874206976672384 20260212.2942 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:37:49.74 +72:49:37.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.70,0.05,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 20260212.2942 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:11.39 +67:01:23.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.48 05:56:04.67 +70:14:12.8
143.51076 20.92459 galactic Cam Second-epoch detections are separated by 1.4" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 485182084399634304 | 05:56:04.67 +70:14:12.8 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.394+/-0.038 (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
Large-amplitude variable Gaia DR2 485182084399634304,2461083.7942,13.48,0.05,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
Large-amplitude variable Gaia DR2 485182084399634304 20260212.2942 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:04.67 +70:14:12.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 550012725949488768,2461083.7942,13.70,0.05,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
Gaia DR3 550012725949488768 20260212.2942 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:57.53 +74:11:24.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.59 05:31:24.44 +64:40:05.9
147.70489 16.37089 galactic Cam Second-epoch detections are separated by 0.8" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J082.8524+64.6796 | 05:31:24.44 +64:40:05.9 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.473+/-0.042 (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
ATO J082.8524+64.6796,2461083.7942,13.59,0.05,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
ATO J082.8524+64.6796 20260212.2942 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:31:24.44 +64:40:05.9 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.47 04:09:07.71 +72:38:02.6
136.51953 15.21302 galactic Cam Second-epoch detections are separated by 1.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:09:07.71 +72:38:02.6 (user input) | T | P | (position from user input) J-Ks=0.352+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:09:07.71 +72:38:02.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.59 05:19:26.63 +71:43:15.1
140.70025 18.89967 galactic Cam Second-epoch detections are separated by 1.3" and 5.4 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 | target | 05:19:26.63 +71:43:15.1 (user input) | T | P | (position from user input) J-Ks=0.782+/-0.038 (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,2461083.7942,13.59,0.05,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 20260212.2942 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:19:26.63 +71:43:15.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.61 05:12:56.01 +64:55:32.5
146.41706 14.82373 galactic Cam Second-epoch detections are separated by 1.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 479268773429926656 | 05:13:00.33 +64:55:17.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.357+/-0.051 (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
Gaia DR3 479268773429926656,2461083.7942,13.61,0.05,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
Gaia DR3 479268773429926656 20260212.2942 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:12:56.01 +64:55:32.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.51 03:32:37.82 +67:01:40.1
137.73549 8.91115 galactic Cam Second-epoch detections are separated by 3.8" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:32:37.82 +67:01:40.1 (user input) | T | P | (position from user input) J-Ks=0.587+/-0.033 (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,2461083.7942,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:32:37.82 +67:01:40.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.68 05:27:07.73 +72:06:05.0
140.65527 19.60591 galactic Cam Second-epoch detections are separated by 1.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:27:07.73 +72:06:05.0 (user input) | T | P | (position from user input) J-Ks=0.665+/-0.035 (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,2461083.7942,13.68,0.05,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 20260212.2942 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:27:07.73 +72:06:05.0 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.70 05:16:17.22 +65:08:05.1
146.43368 15.23445 galactic Cam Second-epoch detections are separated by 0.8" and 5.4 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 | target | 05:16:17.22 +65:08:05.1 (user input) | T | P | (position from user input) J-Ks=0.621+/-0.030 (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,2461083.7942,13.70,0.05,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 20260212.2942 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:16:17.22 +65:08:05.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.39 03:29:14.41 +73:23:38.8
133.71473 13.91997 galactic Cas Second-epoch detections are separated by 1.5" 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 | target | 03:29:14.41 +73:23:38.8 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.037 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2942* 03 29 14.41 +73 23 38.8 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:29:14.41 +73:23:38.8 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 495103802454134528,2461083.7942,13.62,0.05,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
Gaia DR3 495103802454134528 20260212.2942 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:01:43.14 +71:19:25.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.66 04:56:17.58 +74:56:41.9
136.88158 19.20894 galactic Cam Second-epoch detections are separated by 0.3" 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 | target | 04:56:17.58 +74:56:41.9 (user input) | T | P | (position from user input) J-Ks=0.447+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.66,0.05,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 20260212.2942 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:17.58 +74:56:41.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.54 04:31:36.79 +68:45:09.4
140.74866 13.89810 galactic Cam Second-epoch detections are separated by 1.5" 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 | Gaia DR3 496573570324869376 | 04:31:31.30 +68:44:47.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.492+/-0.040 (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
Gaia DR3 496573570324869376,2461083.7942,13.54,0.05,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
Gaia DR3 496573570324869376 20260212.2942 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:31:36.79 +68:45:09.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.39 04:37:06.68 +72:47:26.3
137.85639 16.85335 galactic Cam Second-epoch detections are separated by 1.3" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:37:06.68 +72:47:26.3 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.041 (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,2461083.7942,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:37:06.68 +72:47:26.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.60 05:23:14.34 +65:48:38.9
146.22850 16.20320 galactic Cam Second-epoch detections are separated by 4.7" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 480867016660073344 | 05:23:10.62 +65:48:10.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.879+/-0.033 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 480867016660073344,2461083.7942,13.60,0.05,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 480867016660073344 20260212.2942 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:23:14.34 +65:48:38.9 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.55 05:29:57.61 +69:11:16.2
143.48636 18.43112 galactic Cam Second-epoch detections are separated by 0.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 485442084544249216 | 05:29:56.63 +69:11:59.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.443+/-0.040 (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
Gaia DR3 485442084544249216,2461083.7942,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 485442084544249216 20260212.2942 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:57.61 +69:11:16.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.71 04:24:04.82 +74:15:13.5
136.06629 17.10126 galactic Cam Second-epoch detections are separated by 1.6" 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 | target | 04:24:04.82 +74:15:13.5 (user input) | T | P | (position from user input) J-Ks=0.579+/-0.040 (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,2461083.7942,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:04.82 +74:15:13.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.70 05:39:25.07 +64:10:37.1
148.58675 16.89515 galactic Cam Second-epoch detections are separated by 1.0" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:39:25.07 +64:10:37.1 (user input) | T | P | (position from user input) J-Ks=0.321+/-0.047 (F)
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,2461083.7942,13.70,0.05,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 20260212.2942 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:39:25.07 +64:10:37.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.55 05:42:20.01 +64:09:42.7
148.75412 17.16990 galactic Cam Second-epoch detections are separated by 2.1" and 5.6 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 287751367039242880 | 05:42:15.41 +64:09:24.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.452+/-0.050 (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
Gaia DR3 287751367039242880,2461083.7942,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 287751367039242880 20260212.2942 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:42:20.01 +64:09:42.7 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.64 03:16:55.41 +73:53:12.4
132.69089 13.83846 galactic Cas Second-epoch detections are separated by 1.1" 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 | target | 03:16:55.41 +73:53:12.4 (user input) | T | P | (position from user input) J-Ks=0.491+/-0.044 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2942* 03 16 55.41 +73 53 12.4 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.64,0.05,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 20260212.2942 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:16:55.41 +73:53:12.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.54 03:45:53.23 +72:40:39.1
135.15687 14.08971 galactic Cam Second-epoch detections are separated by 0.3" 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 | 03:45:53.23 +72:40:39.1 (user input) | T | P | (position from user input) J-Ks=0.369+/-0.045 (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,2461083.7942,13.54,0.05,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 20260212.2942 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:53.23 +72:40:39.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.78 05:44:37.98 +73:20:10.6
140.07893 21.31484 galactic Cam Second-epoch detections are separated by 5.1" and 5.4 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 | target | 05:44:37.98 +73:20:10.6 (user input) | T | P | (position from user input) J-Ks=0.335+/-0.049 (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,2461083.7942,13.78,0.05,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 20260212.2942 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:44:37.98 +73:20:10.6 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 480527920400518784,2461083.7942,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480527920400518784 20260212.2942 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:48.92 +66:28:26.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.53 03:35:34.12 +69:25:03.1
136.53028 11.00301 galactic Cas Second-epoch detections are separated by 2.4" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:35:34.12 +69:25:03.1 (user input) | T | P | (position from user input) J-Ks=0.440+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2942* 03 35 34.12 +69 25 03.1 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.53,0.05,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 20260212.2942 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:35:34.12 +69:25:03.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.61 04:30:07.39 +73:12:23.1
137.18087 16.72880 galactic Cam Second-epoch detections are separated by 0.4" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:30:07.39 +73:12:23.1 (user input) | T | P | (position from user input) J-Ks=0.762+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.61,0.05,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 20260212.2942 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:30:07.39 +73:12:23.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.59 03:48:35.94 +69:13:56.1
137.57114 11.56421 galactic Cam Second-epoch detections are separated by 2.6" 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 | target | 03:48:35.94 +69:13:56.1 (user input) | T | P | (position from user input) J-Ks=0.491+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.59,0.05,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 20260212.2942 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:35.94 +69:13:56.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.72 04:39:44.78 +68:25:39.7
141.49983 14.25236 galactic Cam Second-epoch detections are separated by 0.5" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:39:44.78 +68:25:39.7 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.043 (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,2461083.7942,13.72,0.05,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 20260212.2942 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:39:44.78 +68:25:39.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.52 04:31:51.47 +68:47:20.7
140.73546 13.93880 galactic Cam Second-epoch detections are separated by 1.8" and 6.1 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 496574090018649856 | 04:31:55.28 +68:47:05.8 (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 496574090018649856,2461083.7942,13.52,0.05,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
Gaia DR3 496574090018649856 20260212.2942 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:31:51.47 +68:47:20.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.67,0.05,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 20260212.2942 13.67CV 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:48:52.85 +68:02:47.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.48,0.05,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 20260212.2942 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:23:00.46 +74:09:13.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.69 05:54:03.79 +68:47:47.7
144.85620 20.20439 galactic Cam Second-epoch detections are separated by 2.2" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:54:03.79 +68:47:47.7 (user input) | T | P | (position from user input) J-Ks=0.473+/-0.049 (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,2461083.7942,13.69,0.05,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 20260212.2942 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:03.79 +68:47:47.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.45 03:41:55.93 +68:36:21.3
137.49189 10.70076 galactic Cam Second-epoch detections are separated by 3.6" 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 | target | 03:41:55.93 +68:36:21.3 (user input) | T | P | (position from user input) J-Ks=0.442+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.45,0.05,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 20260212.2942 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:55.93 +68:36:21.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.66 04:17:23.80 +72:57:01.5
136.73107 15.87061 galactic Cam Second-epoch detections are separated by 2.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:17:23.80 +72:57:01.5 (user input) | T | P | (position from user input) J-Ks=0.476+/-0.042 (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,2461083.7942,13.66,0.05,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 20260212.2942 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:17:23.80 +72:57:01.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.57 06:33:00.92 +72:03:24.2
142.62475 24.31730 galactic Cam Second-epoch detections are separated by 0.7" and 4.6 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 | target | 06:33:00.92 +72:03:24.2 (user input) | T | P | (position from user input) J-Ks=0.696+/-0.034 (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,2461083.7942,13.57,0.05,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 20260212.2942 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:33:00.92 +72:03:24.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.53 03:20:23.08 +73:29:18.2
133.12513 13.63885 galactic Cas Second-epoch detections are separated by 1.7" 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 | 03:20:23.08 +73:29:18.2 (user input) | T | P | (position from user input) J-Ks=0.447+/-0.045 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2942* 03 20 23.08 +73 29 18.2 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.53,0.05,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 20260212.2942 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:20:23.08 +73:29:18.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.55 04:56:17.99 +74:32:46.5
137.23013 18.98424 galactic Cam Second-epoch detections are separated by 1.9" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:17.99 +74:32:46.5 (user input) | T | P | (position from user input) J-Ks=0.387+/-0.049 (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,2461083.7942,13.55,0.05,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 20260212.2942 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:17.99 +74:32:46.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.59 04:36:00.66 +66:19:30.6
142.91328 12.62154 galactic Cam Second-epoch detections are separated by 0.2" 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 | target | 04:36:00.66 +66:19:30.6 (user input) | T | P | (position from user input) J-Ks=0.426+/-0.047 (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,2461083.7942,13.59,0.05,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 20260212.2942 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:36:00.66 +66:19:30.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.79 04:35:14.02 +73:59:21.8
136.79634 17.50859 galactic Cam Second-epoch detections are separated by 1.4" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:35:14.02 +73:59:21.8 (user input) | T | P | (position from user input) J-Ks=0.308+/-0.046 (F)
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,2461083.7942,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:35:14.02 +73:59:21.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.55 03:21:28.87 +73:21:25.5
133.26711 13.57317 galactic Cas Second-epoch detections are separated by 0.9" and 6.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:21:28.87 +73:21:25.5 (user input) | T | P | (position from user input) J-Ks=0.805+/-0.037 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 12.2942* 03 21 28.87 +73 21 25.5 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.55,0.05,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 20260212.2942 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:21:28.87 +73:21:25.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.63 05:07:09.90 +71:01:44.5
140.78234 17.70251 galactic Cam Second-epoch detections are separated by 3.9" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:07:09.90 +71:01:44.5 (user input) | T | P | (position from user input) J-Ks=0.468+/-0.055 (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,2461083.7942,13.63,0.05,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 20260212.2942 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:09.90 +71:01:44.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.70 06:07:07.49 +71:41:35.8
142.39074 22.28356 galactic Cam Second-epoch detections are separated by 3.8" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:07:07.49 +71:41:35.8 (user input) | T | P | (position from user input) J-Ks=0.421+/-0.038 (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,2461083.7942,13.70,0.05,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 20260212.2942 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:07.49 +71:41:35.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.63 05:23:27.55 +69:02:17.9
143.32667 17.85228 galactic Cam Second-epoch detections are separated by 1.3" 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 | target | 05:23:27.55 +69:02:17.9 (user input) | T | P | (position from user input) J-Ks=0.431+/-0.044 (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,2461083.7942,13.63,0.05,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 20260212.2942 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:23:27.55 +69:02:17.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.74 05:51:06.98 +68:31:25.3
145.00798 19.84943 galactic Cam Second-epoch detections are separated by 1.6" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:51:06.98 +68:31:25.3 (user input) | T | P | (position from user input) J-Ks=0.518+/-0.058 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:51:06.98 +68:31:25.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.54,0.05,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 20260212.2942 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:39:40.89 +67:26:56.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.57 04:53:40.39 +72:30:31.2
138.87588 17.66300 galactic Cam Second-epoch detections are separated by 2.7" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 500709799926462848 | 04:53:46.08 +72:30:19.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.622+/-0.037 (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
Gaia DR3 500709799926462848,2461083.7942,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 500709799926462848 20260212.2942 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:53:40.39 +72:30:31.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.62 04:10:06.87 +69:49:16.0
138.60586 13.25603 galactic Cam Second-epoch detections are separated by 2.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:10:06.87 +69:49:16.0 (user input) | T | P | (position from user input) J-Ks=0.513+/-0.034 (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,2461083.7942,13.62,0.05,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 20260212.2942 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:10:06.87 +69:49:16.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.74 06:05:13.45 +72:24:08.9
141.61491 22.38051 galactic Cam Second-epoch detections are separated by 2.0" and 4.5 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 | target | 06:05:13.45 +72:24:08.9 (user input) | T | P | (position from user input) J-Ks=0.281+/-0.050 (F)
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,2461083.7942,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:13.45 +72:24:08.9 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.69 06:03:50.99 +73:04:20.1
140.89491 22.50760 galactic Cam Second-epoch detections are separated by 3.2" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:03:50.99 +73:04:20.1 (user input) | T | P | (position from user input) J-Ks=0.362+/-0.048 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.69,0.05,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 20260212.2942 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:50.99 +73:04:20.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.71 05:39:08.59 +63:44:03.5
148.98067 16.66146 galactic Cam Second-epoch detections are separated by 2.6" and 5.4 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 | target | 05:39:08.59 +63:44:03.5 (user input) | T | P | (position from user input) J-Ks=0.453+/-0.046 (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,2461083.7942,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:39:08.59 +63:44:03.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.63 06:09:47.66 +70:46:43.2
143.40020 22.18618 galactic Cam Second-epoch detections are separated by 0.8" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:09:47.66 +70:46:43.2 (user input) | T | P | (position from user input) J-Ks=0.590+/-0.037 (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,2461083.7942,13.63,0.05,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 20260212.2942 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:09:47.66 +70:46:43.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.77 06:05:30.63 +67:02:43.0
147.01952 20.53524 galactic Cam Second-epoch detections are separated by 0.7" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:05:30.63 +67:02:43.0 (user input) | T | P | (position from user input) J-Ks=0.575+/-0.043 (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,2461083.7942,13.77,0.05,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 20260212.2942 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:30.63 +67:02:43.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.73 05:59:53.80 +73:38:42.1
140.20793 22.43572 galactic Cam Second-epoch detections are separated by 2.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:59:53.80 +73:38:42.1 (user input) | T | P | (position from user input) J-Ks=0.402+/-0.040 (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,2461083.7942,13.73,0.05,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 20260212.2942 13.73CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:53.80 +73:38:42.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.80 05:53:35.29 +73:35:24.6
140.09178 22.00063 galactic Cam Second-epoch detections are separated by 0.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:53:35.29 +73:35:24.6 (user input) | T | P | (position from user input) J-Ks=0.429+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.80,0.05,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 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:35.29 +73:35:24.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.82 04:56:17.86 +70:32:23.6
140.67940 16.68818 galactic Cam Second-epoch detections are separated by 1.3" and 5.4 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 | target | 04:56:17.86 +70:32:23.6 (user input) | T | P | (position from user input) J-Ks=0.429+/-0.046 (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,2461083.7942,13.82,0.05,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 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:17.86 +70:32:23.6 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.64,0.05,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 20260212.2942 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:14:31.06 +70:43:07.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.81 05:58:04.61 +72:58:26.4
140.83751 22.07817 galactic Cam Second-epoch detections are separated by 1.4" and 4.6 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 | target | 05:58:04.61 +72:58:26.4 (user input) | T | P | (position from user input) J-Ks=0.739+/-0.034 (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,2461083.7942,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:04.61 +72:58:26.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.52 05:28:18.47 +70:24:25.6
142.28293 18.88608 galactic Cam Second-epoch detections are separated by 0.9" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 485797707835499904 | 05:28:22.64 +70:25:06.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.462+/-0.043 (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
Gaia DR3 485797707835499904,2461083.7942,13.52,0.05,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
Gaia DR3 485797707835499904 20260212.2942 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:28:18.47 +70:24:25.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.62,0.05,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 20260212.2942 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:12:37.92 +64:29:47.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.61 05:12:13.95 +64:51:32.3
146.43256 14.72495 galactic Cam Second-epoch detections are separated by 1.6" and 5.6 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 | target | 05:12:13.95 +64:51:32.3 (user input) | T | P | (position from user input) J-Ks=0.403+/-0.045 (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,2461083.7942,13.61,0.05,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 20260212.2942 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:12:13.95 +64:51:32.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.77 05:56:55.39 +71:35:45.3
142.18655 21.49709 galactic Cam Second-epoch detections are separated by 0.3" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:56:55.39 +71:35:45.3 (user input) | T | P | (position from user input) J-Ks=0.602+/-0.037 (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,2461083.7942,13.77,0.05,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 20260212.2942 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:56:55.39 +71:35:45.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.54 03:54:53.76 +74:53:41.2
134.16166 16.18424 galactic Cam Second-epoch detections are separated by 3.0" and 5.4 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 | target | 03:54:53.76 +74:53:41.2 (user input) | T | P | (position from user input) J-Ks=0.613+/-0.034 (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,2461083.7942,13.54,0.05,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 20260212.2942 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:53.76 +74:53:41.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.69 05:34:04.47 +64:45:42.1
147.76403 16.66520 galactic Cam Second-epoch detections are separated by 0.5" and 5.4 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 | target | 05:34:04.47 +64:45:42.1 (user input) | T | P | (position from user input) J-Ks=0.668+/-0.039 (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,2461083.7942,13.69,0.05,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 20260212.2942 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:04.47 +64:45:42.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.71 05:29:38.37 +70:26:14.6
142.31061 18.99867 galactic Cam Second-epoch detections are separated by 1.2" 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 | Large-amplitude variable Gaia DR2 485800868927773952 | 05:29:38.37 +70:26:14.6 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.454+/-0.040 (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
Large-amplitude variable Gaia DR2 485800868927773952,2461083.7942,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 485800868927773952 20260212.2942 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:38.37 +70:26:14.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.75 04:42:28.06 +68:36:51.9
141.51333 14.56341 galactic Cam Second-epoch detections are separated by 0.3" and 5.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:42:28.06 +68:36:51.9 (user input) | T | P | (position from user input) J-Ks=0.437+/-0.042 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.75,0.05,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 20260212.2942 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:42:28.06 +68:36:51.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.68 05:16:13.49 +71:25:50.1
140.82861 18.53338 galactic Cam Second-epoch detections are separated by 0.9" and 5.4 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 498063893914090752 | 05:16:12.40 +71:26:30.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.641+/-0.039 (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
Gaia DR3 498063893914090752,2461083.7942,13.68,0.05,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
Gaia DR3 498063893914090752 20260212.2942 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:16:13.49 +71:25:50.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461083.7942,13.78,0.05,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 20260212.2942 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:39.77 +71:19:17.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.72 05:47:40.79 +66:13:52.4
147.06672 18.59025 galactic Cam Second-epoch detections are separated by 0.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:47:40.79 +66:13:52.4 (user input) | T | P | (position from user input) J-Ks=0.363+/-0.057 (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,2461083.7942,13.72,0.05,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 20260212.2942 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:47:40.79 +66:13:52.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.78 05:26:02.10 +66:01:33.7
146.18590 16.55816 galactic Cam Second-epoch detections are separated by 1.8" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 480829049149046272 | 05:26:03.97 +66:00:58.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.581+/-0.040 (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
Gaia DR3 480829049149046272,2461083.7942,13.78,0.05,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
Gaia DR3 480829049149046272 20260212.2942 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:26:02.10 +66:01:33.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.76 05:34:57.16 +70:26:59.4
142.51653 19.39869 galactic Cam Second-epoch detections are separated by 2.4" 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 | target | 05:34:57.16 +70:26:59.4 (user input) | T | P | (position from user input) J-Ks=0.637+/-0.037 (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,2461083.7942,13.76,0.05,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 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:34:57.16 +70:26:59.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.71 03:53:54.20 +71:11:43.5
136.62798 13.35501 galactic Cam Second-epoch detections are separated by 2.3" 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 | target | 03:53:54.20 +71:11:43.5 (user input) | T | P | (position from user input) J-Ks=0.505+/-0.057 (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,2461083.7942,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260212.2942 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:54.20 +71:11:43.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.62 04:05:44.86 +75:02:48.9
134.59064 16.77478 galactic Cam Second-epoch detections are separated by 4.1" 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 | target | 04:05:44.86 +75:02:48.9 (user input) | T | P | (position from user input) J-Ks=0.325+/-0.043 (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,2461083.7942,13.62,0.05,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 20260212.2942 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:05:44.86 +75:02:48.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.85 05:36:31.68 +64:13:37.6
148.38590 16.64140 galactic Cam Second-epoch detections are separated by 1.4" 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 | target | 05:36:31.68 +64:13:37.6 (user input) | T | P | (position from user input) J-Ks=0.487+/-0.042 (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,2461083.7942,13.85,0.05,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 20260212.2942 13.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:36:31.68 +64:13:37.6 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.68 05:07:01.17 +73:43:57.8
138.37485 19.14942 galactic Cam Second-epoch detections are separated by 1.9" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:07:01.17 +73:43:57.8 (user input) | T | P | (position from user input) J-Ks=0.557+/-0.038 (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,2461083.7942,13.68,0.05,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 20260212.2942 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:01.17 +73:43:57.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 287763053647372416,2461083.7942,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 287763053647372416 20260212.2942 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:41:47.60 +64:19:31.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 495611742466826240,2461083.7942,13.68,0.05,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
Gaia DR3 495611742466826240 20260212.2942 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:37:00.33 +67:41:14.3 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.80 04:54:03.20 +71:36:09.4
139.66543 17.15880 galactic Cam Second-epoch detections are separated by 2.6" 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 | target | 04:54:03.20 +71:36:09.4 (user input) | T | P | (position from user input) J-Ks=0.465+/-0.049 (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,2461083.7942,13.80,0.05,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 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:54:03.20 +71:36:09.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.89 04:55:03.40 +73:08:18.3
138.39810 18.11052 galactic Cam Second-epoch detections are separated by 3.1" and 5.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:55:03.40 +73:08:18.3 (user input) | T | P | (position from user input) J-Ks=0.626+/-0.035 (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,2461083.7942,13.89,0.05,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 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:55:03.40 +73:08:18.3 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.65 03:51:41.54 +72:30:41.4
135.61017 14.24084 galactic Cam Second-epoch detections are separated by 2.9" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:51:41.54 +72:30:41.4 (user input) | T | P | (position from user input) J-Ks=0.668+/-0.035 (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,2461083.7942,13.65,0.05,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 20260212.2942 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:41.54 +72:30:41.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.64 03:54:25.44 +67:41:53.2
138.99219 10.73049 galactic Cam Second-epoch detections are separated by 0.3" and 6.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:54:25.44 +67:41:53.2 (user input) | T | P | (position from user input) J-Ks=0.389+/-0.036 (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,2461083.7942,13.64,0.05,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 20260212.2942 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:54:25.44 +67:41:53.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 12.2942 2461083.7942 13.80 04:12:18.90 +66:10:04.5
141.35880 10.77829 galactic Cam Second-epoch detections are separated by 2.9" 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 | target | 04:12:18.90 +66:10:04.5 (user input) | T | P | (position from user input) J-Ks=0.554+/-0.033 (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,2461083.7942,13.80,0.05,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 20260212.2942 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_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:12:18.90 +66:10:04.5 ;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_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 2175705,2461083.7942,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS 2175705 20260212.2942 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:44.03 +67:40:08.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20_00sec_-14_90C_LIGHT_0309_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20_00sec_-15_00C_LIGHT_0308_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: 2461083.79455243 12.02.2026 07:03:59.330 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 7
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 5 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 15922
Objects passed selection criteria: 15915
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 15383.5
Average stars matched: 15049.8 (97.8305 %)
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 Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Feb 12 01:08:40 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
First image: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Last image: 2461083.79455243 12.02.2026 07:03:59.330 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 249
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: 54 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): 113819
Objects passed selection criteria: 113523
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: 109569
Average stars matched: 105503 (96.2891 %)
Memory usage VmPeak: 1936068 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Feb 12 01:10:40 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
SExtractor catalog cache: saved Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat to cache
SExtractor catalog cache: saved Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.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: 2461083.79377507
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_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits'
wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.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 04:48:07.339 +69:59:40.50
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:47:48.196 +70:00:29.12
Second-epoch image center 04:48:09.269 +69:59:08.97
Angular distance between the image centers 0.04 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 04:48:07.339 +69:59:40.50
Second-epoch second image center 04:48:09.269 +69:59:08.97
Angular distance between the image centers 0.00918 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.JIiHYjQes9
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.xAmM6F3qjZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits &> /tmp/tmp.PzUHRrpvfH
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits &> /tmp/tmp.kvQlYDaJDT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Found non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
The reference image (wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits) and catalog (wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat) found
'wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 58 out of 16183 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.881698
a=0.000000 b=1.000000 c=22.881698
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.26
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.26
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 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
2.0 pix fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
2.0 pix fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
Limiting magnitude estimates:
15.3 mag. Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
15.2 mag. Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
15.2 mag. fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
15.2 mag. fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
All-image limiting magnitude estimate: 15.2 (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 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.JIiHYjQes9 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/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.xAmM6F3qjZ (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/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.PzUHRrpvfH (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
Checking if the catalog wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
WCS catalog name: wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1174, passed=14782
Got 14782 stars (including 13593 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits.cat
util/solve_plate_with_UCAC5 got 14782 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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 970 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: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.36"
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 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.36"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 969 stars left (next iteration limit 1065)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits -region wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.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.kvQlYDaJDT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
Checking if the catalog wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
WCS catalog name: wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1110, passed=14719
Got 14719 stars (including 13587 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits.cat
util/solve_plate_with_UCAC5 got 14719 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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: 0.38"
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 969 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: 0.34"
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_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits -region wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits'
Saving fully-calibrated image wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits'
Preparing the HTML report for the field Cam-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21021.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21055.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21070.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21072.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21077.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21091.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
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: 0s
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21021_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 21021_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 04:32:14.80 +73:00:38.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.606 501621325127748224 068.06184932149 +73.01077076149 12.2280 11.6879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.606#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21055_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 21055_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 05:24:53.48 +64:43:48.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.61, MAG_FAINT_SEARCH_LIMIT=12.59)GAIADR2_OUTPUT=# 0.256 479952600942151680 081.22266683122 +64.73022403311 11.7000 11.2253 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.256#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21063_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 21063_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 03:41:24.22 +72:39:24.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21070_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 21070_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 05:20:10.36 +71:33:54.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.09, MAG_FAINT_SEARCH_LIMIT=13.07)GAIADR2_OUTPUT=# 0.989 498147899176343936 080.04274431906 +71.56495450163 11.8098 11.0125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.989#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21072_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 21072_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 04:50:20.66 +68:09:06.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.12, MAG_FAINT_SEARCH_LIMIT=13.10)GAIADR2_OUTPUT=# 0.655 495967984234117504 072.58584113756 +68.15164736946 12.0959 11.3506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.655#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21077_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 21077_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 05:15:02.74 +73:00:52.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.24, MAG_FAINT_SEARCH_LIMIT=13.22)GAIADR2_OUTPUT=# 0.466 499272768290947328 078.76097407482 +73.01458988992 12.0140 11.2520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.466#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21091_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 21091_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 05:04:24.10 +69:47:49.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.547 496231587848912128 076.10027246800 +69.79728243252 12.0807 11.4351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.547#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
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 ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
SExtractor catalog cache: saved Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat to cache
SExtractor catalog cache: saved Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Creating symlink local_wcs_cache/wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits exists and is non-empty
wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits exists and is non-empty
wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits exists and is non-empty
wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.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 04:48:07.339 +69:59:40.50
Angular distance between the image centers 0.03 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:47:48.196 +70:00:29.12
Second-epoch image center 04:48:09.269 +69:59:08.97
Angular distance between the image centers 0.04 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 04:48:07.339 +69:59:40.50
Second-epoch second image center 04:48:09.269 +69:59:08.97
Angular distance between the image centers 0.00918 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.3ISrMFkZEl
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.bXXRaSnzXr
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits &> /tmp/tmp.rXYhShIROU
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits &> /tmp/tmp.uxdbXCmEiq
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Found non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
The reference image (wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits) and catalog (wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat) found
'wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 85 out of 113524 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 21.485425
a=0.000000 b=1.000000 c=21.485425
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.18
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.18
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 231 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
1.9 pix Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
1.8 pix fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
1.9 pix fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
Limiting magnitude estimates:
14.2 mag. Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
14.2 mag. Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
14.1 mag. fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
14.1 mag. fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.3ISrMFkZEl (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/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.bXXRaSnzXr (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/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.rXYhShIROU (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
Checking if the catalog wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
WCS catalog name: wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=30, blended=8287, passed=107378
Got 107378 stars (including 98940 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits.cat
util/solve_plate_with_UCAC5 got 107378 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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: 0.38"
Estimated accuracy of the plate solution: 0.38"
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_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits -region wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.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.uxdbXCmEiq (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
Checking if the catalog wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
WCS catalog name: wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=40, blended=8257, passed=106977
Got 106977 stars (including 98554 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits.cat
util/solve_plate_with_UCAC5 got 106977 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.8'
Seting catalog search parameters based on the expected field of view 941.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013081 (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 0.010464 (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: 0.39"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
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: 0.38"
Estimated accuracy of the plate solution: 0.37"
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_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits -region wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-02-52_20.00sec_-15.00C_LIGHT_0308.fits
Saving fully-calibrated image wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-12_CI_Cam-06-Q1b1x1_010619_TTUQ1b1x1_4354_8UD9NOFz/wcs_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309.fits
Preparing the HTML report for the field Cam-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out133183.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133483.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133796.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133915.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133934.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133979.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134152.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134261.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134296.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134338.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out107095.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133027.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133028.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133032.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133035.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133047.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133055.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133059.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133075.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133099.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133102.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133103.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133107.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133118.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133122.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133130.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133142.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133291.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133315.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133369.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133389.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133393.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133419.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133436.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133452.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133462.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133489.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133499.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133507.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133514.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133516.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133518.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133540.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133560.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133561.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133566.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133568.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133574.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133607.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133630.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133644.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133647.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133663.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133667.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133668.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133669.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133678.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133679.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133680.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133701.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133706.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133712.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133716.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133721.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133733.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133739.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133742.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133791.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133793.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133795.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133797.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133802.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133803.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133807.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133808.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133809.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133813.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133816.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133818.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133820.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133827.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133829.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133836.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133840.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133846.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133852.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133856.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133858.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133863.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133875.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133877.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133879.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133886.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133892.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133893.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133898.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133902.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133905.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133910.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133911.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133913.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133917.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133920.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133921.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133923.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133929.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133930.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133932.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133933.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133936.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133938.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133946.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133953.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133958.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133964.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133967.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133968.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133982.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133994.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134009.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134013.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134014.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134022.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134036.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134041.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134043.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134048.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134053.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134054.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134060.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134067.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134079.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134081.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134083.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134094.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134109.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134123.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134126.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134131.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134136.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134154.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134156.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134159.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134163.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134169.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134176.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134181.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134186.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134199.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134200.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134202.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134206.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134207.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134213.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134232.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134240.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134247.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134253.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134258.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134282.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134297.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134316.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134348.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 268s
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: 117s
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Considering the candidate 133025_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133025_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133027_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133027_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133028_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133028_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133032_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133032_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133035_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133035_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133043_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133043_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 05:57:22.10 +65:29:48.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133047_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133047_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133055_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133055_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133056_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133056_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133059_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133059_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133060_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133060_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133075_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133075_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133076_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133076_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133080_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133080_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 04:28:35.68 +73:35:59.6 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133099_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133099_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133102_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133102_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133103_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133103_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133105_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133105_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133107_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133107_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133108_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133108_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133112_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133112_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133118_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133118_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133121_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133121_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133122_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133122_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133123_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133123_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133124_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133124_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133130_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133130_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133131_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133131_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133136_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133136_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133140_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133140_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133142_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133142_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133183_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133183_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 05:30:08.12 +67:13:51.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.70, MAG_FAINT_SEARCH_LIMIT=11.68)GAIADR2_OUTPUT=# 0.322 481264455755828608 082.53381310963 +67.23097796096 11.5859 10.6706 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.322#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133239_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133239_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 04:13:40.79 +72:09:24.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133252_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133252_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133284_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133284_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 04:13:32.37 +72:06:03.2 in the exclusion list exclusion_list_bsc.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133291_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133291_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133315_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133315_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133320_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133320_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133347_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133347_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 04:10:08.93 +68:21:09.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133365_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133365_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133369_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133369_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133382_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133382_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 05:05:47.05 +73:00:51.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133389_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133389_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133393_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133393_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133418_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133418_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 03:29:09.12 +72:34:17.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133419_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133419_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133421_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133421_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 03:57:23.95 +71:25:01.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133436_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133436_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133444_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133444_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 05:44:28.78 +64:32:52.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133452_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133452_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133462_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133462_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133473_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133473_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133483_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133483_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 03:22:08.34 +68:55:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.91, MAG_FAINT_SEARCH_LIMIT=13.89)GAIADR2_OUTPUT=# 3.921 493107020618961280 050.53193565403 +68.92543044173 13.8197 12.7427 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133489_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133489_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133499_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133499_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133501_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133501_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 05:04:29.75 +65:50:11.7 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133503_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133503_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 04:16:55.53 +69:09:49.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133507_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133507_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133514_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133514_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133516_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133516_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133518_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133518_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133540_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133540_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133556_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133556_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133560_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133560_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133561_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133561_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133566_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133566_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133568_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133568_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133573_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133573_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133574_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133574_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133599_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133599_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133607_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133607_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133612_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133612_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 05:12:25.16 +64:18:56.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133630_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133630_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133644_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133644_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133645_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133645_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133647_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133647_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133663_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133663_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133667_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133667_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133668_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133668_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133669_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133669_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133678_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133678_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133679_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133679_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133680_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133680_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133682_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133682_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 03:38:54.32 +72:20:33.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133701_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133701_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133706_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133706_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133712_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133712_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133716_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133716_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133719_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133719_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133721_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133721_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133733_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133733_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133739_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133739_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133742_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133742_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133786_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133786_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133791_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133791_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133793_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133793_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133795_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133795_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133796_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133796_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 04:17:15.70 +66:57:56.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 2.089 489701042833419648 064.31682306768 +66.96573963736 12.3157 10.3326 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.089#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133797_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133797_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133802_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133802_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133803_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133803_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133807_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133807_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133808_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133808_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133809_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133809_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133813_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133813_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133816_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133816_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133818_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133818_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133820_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133820_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133827_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133827_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133829_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133829_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133833_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133833_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133836_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133836_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133840_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133840_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133845_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133845_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133846_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133846_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133852_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133852_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133853_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133853_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133856_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133856_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133858_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133858_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133863_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133863_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133867_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133867_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133875_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133875_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133877_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133877_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133879_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133879_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133881_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133881_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133883_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133883_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 03:43:33.23 +70:59:16.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133886_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133886_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133892_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133892_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133893_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133893_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133898_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133898_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133902_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133902_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133905_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133905_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133910_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133910_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133911_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133911_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133913_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133913_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133915_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133915_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 03:21:16.45 +71:23:02.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.44, MAG_FAINT_SEARCH_LIMIT=14.42)GAIADR2_OUTPUT=# 0.798 543098820737797120 050.31899394077 +71.38397075451 14.3341 13.4182 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.798#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133917_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133917_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133920_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133920_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133921_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133921_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133923_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133923_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133929_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133929_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133930_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133930_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133932_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133932_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133933_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133933_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133934_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133934_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 06:19:03.59 +69:48:39.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.64, MAG_FAINT_SEARCH_LIMIT=14.62)GAIADR2_OUTPUT=# 1.462 1107017860519213440 094.76388767844 +69.81072028033 14.6166 13.9103 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.462#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133936_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133936_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133938_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133938_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133946_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133946_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133950_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133950_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133951_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133951_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133953_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133953_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133958_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133958_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133960_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133960_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133964_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133964_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133967_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133967_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133968_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133968_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133979_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 133979_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 04:01:41.60 +70:12:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.51, MAG_FAINT_SEARCH_LIMIT=14.49)GAIADR2_OUTPUT=# 0.842 494224193151834496 060.42391281977 +70.21668301171 14.4545 13.5481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.842#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133981_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133981_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133982_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133982_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133986_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133986_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133989_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133989_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133994_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 133994_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134007_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134007_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134009_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134009_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134013_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134013_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134014_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134014_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134018_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134018_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134022_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134022_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134023_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134023_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134030_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 134030_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 03:54:25.21 +65:04:22.9 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134036_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134036_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134041_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134041_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134043_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134043_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134048_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134048_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134053_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134053_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134054_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134054_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134060_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134060_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134064_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134064_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134067_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134067_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134069_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134069_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134078_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134078_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134079_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134079_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134081_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134081_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134083_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134083_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134094_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134094_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134109_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134109_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134123_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134123_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134124_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 134124_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 04:02:09.62 +70:45:38.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134126_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134126_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134131_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134131_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134136_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134136_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134140_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134140_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134141_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134141_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134146_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134146_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134148_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134148_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134150_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134150_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134152_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 134152_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 05:10:59.08 +66:29:25.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.80, MAG_FAINT_SEARCH_LIMIT=14.78)GAIADR2_OUTPUT=# 0.066 482648534736468480 077.74612950347 +66.49053852153 14.7527 14.2249 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.066#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134153_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134153_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134154_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134154_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134156_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134156_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134159_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134159_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134163_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134163_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134169_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134169_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134176_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134176_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134181_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134181_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134186_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134186_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134199_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134199_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134200_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134200_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134202_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134202_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134204_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134204_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134206_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134206_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134207_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134207_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134213_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134213_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134224_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134224_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134232_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134232_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134240_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134240_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134247_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134247_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134253_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134253_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134258_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134258_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134259_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134259_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134261_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 134261_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 05:00:36.96 +65:21:04.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.67, MAG_FAINT_SEARCH_LIMIT=14.65)GAIADR2_OUTPUT=# 0.600 482460140291139456 075.15375840635 +65.35100621885 14.5280 13.6736 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.600#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134280_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134280_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134282_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134282_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134296_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 134296_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 03:41:56.02 +71:44:40.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 0.374 543333330249889152 055.48336026849 +71.74436978738 14.4371 13.3924 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.374#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134297_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134297_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134316_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134316_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134338_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 134338_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 03:44:10.77 +70:00:10.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 0.457 494730690054975488 056.04457321923 +70.00299035317 14.6216 13.7427 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.457#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134348_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 134348_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77457_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 77457_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 03:41:04.03 +67:38:52.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90043_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
The candidate 90043_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309 did not pass the final checks
**** FOUND 04:05:39.15 +66:19:55.1 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 107095_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
Preparing report for the candidate 107095_fd_Cam-06-Q1b1x1_2026-02-12_01-03-59_20.00sec_-14.90C_LIGHT_0309
make_report_in_HTML.sh Phase 2 (HTML assembly): 33s
make_report_in_HTML.sh TOTAL: 418s
Prepared the HTML report for the field Cam-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:56:44.03 +67:40:08.8
05:25:42.43 +72:10:43.5
05:03:00.83 +71:37:27.5
05:48:21.87 +64:32:09.8
05:03:11.35 +69:43:42.8
05:03:18.16 +72:39:59.7
04:20:25.52 +74:02:55.8
04:33:03.65 +69:49:45.6
04:06:37.63 +68:36:19.4
05:25:12.41 +66:12:18.6
04:56:22.40 +72:43:26.7
04:55:22.27 +66:47:32.8
05:59:14.60 +70:12:05.1
04:49:37.46 +69:17:39.2
04:28:13.58 +68:28:43.7
05:15:55.15 +73:39:59.9
06:14:59.89 +70:38:32.0
05:01:49.26 +66:03:52.6
05:34:40.32 +67:06:25.9
04:54:19.78 +68:57:49.3
05:02:53.80 +65:01:14.0
04:32:28.63 +67:14:24.4
04:02:19.72 +70:42:08.6
05:38:34.63 +70:25:44.9
05:13:00.11 +68:41:29.0
03:24:31.89 +70:39:05.7
05:44:46.41 +64:00:07.9
05:27:07.63 +72:34:27.7
05:52:27.86 +70:32:03.8
03:45:58.83 +68:00:22.9
04:42:14.62 +69:04:10.2
04:57:37.94 +70:38:34.8
04:48:51.80 +74:27:59.9
05:32:38.74 +71:28:25.8
05:38:30.12 +74:15:31.5
05:45:07.80 +70:54:04.3
05:51:35.41 +68:00:53.7
03:37:05.47 +69:37:35.6
05:17:15.82 +73:34:58.5
05:48:53.23 +73:08:42.4
05:42:16.32 +68:55:14.9
04:03:46.01 +74:47:17.6
04:24:07.64 +66:28:21.7
04:41:23.25 +72:55:31.7
04:49:57.56 +67:08:31.1
03:34:59.11 +71:38:54.0
04:46:14.94 +66:27:36.0
03:58:46.26 +73:22:06.9
05:53:04.13 +64:13:56.7
04:29:18.98 +69:31:54.8
04:20:01.28 +68:13:24.2
04:54:50.65 +66:57:16.2
05:51:22.12 +64:43:30.3
05:02:57.10 +65:09:02.1
05:15:57.20 +70:34:25.2
06:25:10.05 +70:16:23.9
05:26:37.67 +64:37:46.4
05:36:37.21 +74:18:46.1
05:54:33.59 +72:46:27.0
05:01:18.34 +66:42:39.3
03:35:57.74 +72:27:17.7
04:47:41.50 +69:27:47.8
05:36:57.85 +65:42:05.7
05:51:19.03 +72:42:38.2
05:38:13.79 +68:50:54.9
04:45:29.78 +74:16:14.4
06:28:02.54 +72:19:51.9
05:44:29.09 +70:20:34.0
04:40:44.25 +69:05:34.4
04:49:42.22 +75:05:48.9
04:24:13.15 +67:07:08.2
04:30:44.57 +74:12:33.4
04:54:16.84 +65:21:23.2
03:20:24.91 +70:25:30.5
04:41:44.13 +74:34:43.8
06:14:38.82 +70:39:51.6
04:53:44.19 +74:47:25.4
05:14:05.29 +70:19:07.5
05:11:19.59 +72:08:05.9
05:33:39.65 +64:23:07.4
05:24:32.25 +69:38:25.8
03:20:56.37 +71:13:17.8
05:50:23.86 +67:00:17.6
03:42:15.16 +71:59:39.0
04:24:34.43 +69:53:54.5
04:32:13.20 +69:46:33.9
03:41:25.57 +68:24:22.9
05:07:08.88 +65:22:12.0
03:36:50.18 +72:50:03.8
03:25:13.90 +73:15:13.9
06:07:10.79 +71:30:10.3
05:36:48.01 +64:22:23.6
06:10:05.98 +69:59:13.0
04:09:14.33 +70:14:49.4
03:56:03.36 +69:57:43.5
05:22:05.63 +66:32:17.4
03:37:19.76 +67:04:59.2
03:53:39.59 +67:23:17.3
05:19:37.55 +70:19:20.9
05:18:23.35 +72:55:11.7
05:11:29.94 +74:28:23.6
03:33:02.07 +68:48:58.5
05:45:03.32 +65:00:23.3
03:25:02.01 +73:22:53.5
05:06:40.14 +64:59:44.7
04:10:48.95 +74:38:56.2
03:43:52.01 +74:14:46.5
04:18:40.06 +75:11:20.7
05:31:19.79 +67:14:13.2
05:29:51.31 +72:20:59.5
04:21:07.90 +66:11:01.9
05:13:28.28 +65:11:51.8
04:54:44.77 +65:04:13.6
03:55:47.22 +71:26:44.6
03:22:47.79 +73:32:35.9
03:53:52.72 +67:13:28.9
04:25:22.03 +65:57:39.5
05:34:52.29 +63:51:44.1
05:16:24.61 +64:47:32.3
05:35:04.26 +72:27:17.1
04:24:11.80 +67:34:12.8
04:37:49.74 +72:49:37.5
05:54:11.39 +67:01:23.8
05:56:04.67 +70:14:12.8
04:25:57.53 +74:11:24.2
05:31:24.44 +64:40:05.9
04:09:07.71 +72:38:02.6
05:19:26.63 +71:43:15.1
05:12:56.01 +64:55:32.5
03:32:37.82 +67:01:40.1
05:27:07.73 +72:06:05.0
05:16:17.22 +65:08:05.1
03:29:14.41 +73:23:38.8
04:01:43.14 +71:19:25.4
04:56:17.58 +74:56:41.9
04:31:36.79 +68:45:09.4
04:37:06.68 +72:47:26.3
05:23:14.34 +65:48:38.9
05:29:57.61 +69:11:16.2
04:24:04.82 +74:15:13.5
05:39:25.07 +64:10:37.1
05:42:20.01 +64:09:42.7
03:16:55.41 +73:53:12.4
03:45:53.23 +72:40:39.1
05:44:37.98 +73:20:10.6
05:46:48.92 +66:28:26.6
03:35:34.12 +69:25:03.1
04:30:07.39 +73:12:23.1
03:48:35.94 +69:13:56.1
04:39:44.78 +68:25:39.7
04:31:51.47 +68:47:20.7
04:48:52.85 +68:02:47.7
04:23:00.46 +74:09:13.0
05:54:03.79 +68:47:47.7
03:41:55.93 +68:36:21.3
04:17:23.80 +72:57:01.5
06:33:00.92 +72:03:24.2
03:20:23.08 +73:29:18.2
04:56:17.99 +74:32:46.5
04:36:00.66 +66:19:30.6
04:35:14.02 +73:59:21.8
03:21:28.87 +73:21:25.5
05:07:09.90 +71:01:44.5
06:07:07.49 +71:41:35.8
05:23:27.55 +69:02:17.9
05:51:06.98 +68:31:25.3
03:39:40.89 +67:26:56.5
04:53:40.39 +72:30:31.2
04:10:06.87 +69:49:16.0
06:05:13.45 +72:24:08.9
06:03:50.99 +73:04:20.1
05:39:08.59 +63:44:03.5
06:09:47.66 +70:46:43.2
06:05:30.63 +67:02:43.0
05:59:53.80 +73:38:42.1
05:53:35.29 +73:35:24.6
04:56:17.86 +70:32:23.6
04:14:31.06 +70:43:07.2
05:58:04.61 +72:58:26.4
05:28:18.47 +70:24:25.6
05:12:37.92 +64:29:47.3
05:12:13.95 +64:51:32.3
05:56:55.39 +71:35:45.3
03:54:53.76 +74:53:41.2
05:34:04.47 +64:45:42.1
05:29:38.37 +70:26:14.6
04:42:28.06 +68:36:51.9
05:16:13.49 +71:25:50.1
05:03:39.77 +71:19:17.3
05:47:40.79 +66:13:52.4
05:26:02.10 +66:01:33.7
05:34:57.16 +70:26:59.4
03:53:54.20 +71:11:43.5
04:05:44.86 +75:02:48.9
05:36:31.68 +64:13:37.6
05:07:01.17 +73:43:57.8
05:41:47.60 +64:19:31.1
04:37:00.33 +67:41:14.3
04:54:03.20 +71:36:09.4
04:55:03.40 +73:08:18.3
03:51:41.54 +72:30:41.4
03:54:25.44 +67:41:53.2
04:12:18.90 +66:10:04.5
########### 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 ####
05:25:42.43 +72:10:43.5
05:03:00.83 +71:37:27.5
05:48:21.87 +64:32:09.8
05:03:11.35 +69:43:42.8
05:03:18.16 +72:39:59.7
04:20:25.52 +74:02:55.8
04:33:03.65 +69:49:45.6
04:06:37.63 +68:36:19.4
05:25:12.41 +66:12:18.6
04:56:22.40 +72:43:26.7
04:55:22.27 +66:47:32.8
05:59:14.60 +70:12:05.1
04:49:37.46 +69:17:39.2
04:28:13.58 +68:28:43.7
05:15:55.15 +73:39:59.9
06:14:59.89 +70:38:32.0
05:01:49.26 +66:03:52.6
05:34:40.32 +67:06:25.9
04:54:19.78 +68:57:49.3
05:02:53.80 +65:01:14.0
04:32:28.63 +67:14:24.4
04:02:19.72 +70:42:08.6
05:38:34.63 +70:25:44.9
05:13:00.11 +68:41:29.0
03:24:31.89 +70:39:05.7
05:44:46.41 +64:00:07.9
05:27:07.63 +72:34:27.7
05:52:27.86 +70:32:03.8
03:45:58.83 +68:00:22.9
04:42:14.62 +69:04:10.2
04:57:37.94 +70:38:34.8
04:48:51.80 +74:27:59.9
05:32:38.74 +71:28:25.8
05:38:30.12 +74:15:31.5
05:45:07.80 +70:54:04.3
05:51:35.41 +68:00:53.7
03:37:05.47 +69:37:35.6
05:17:15.82 +73:34:58.5
05:48:53.23 +73:08:42.4
05:42:16.32 +68:55:14.9
04:03:46.01 +74:47:17.6
04:24:07.64 +66:28:21.7
04:41:23.25 +72:55:31.7
04:49:57.56 +67:08:31.1
03:34:59.11 +71:38:54.0
04:46:14.94 +66:27:36.0
03:58:46.26 +73:22:06.9
05:53:04.13 +64:13:56.7
04:29:18.98 +69:31:54.8
04:20:01.28 +68:13:24.2
04:54:50.65 +66:57:16.2
05:51:22.12 +64:43:30.3
05:02:57.10 +65:09:02.1
05:15:57.20 +70:34:25.2
06:25:10.05 +70:16:23.9
05:26:37.67 +64:37:46.4
05:36:37.21 +74:18:46.1
05:54:33.59 +72:46:27.0
05:01:18.34 +66:42:39.3
03:35:57.74 +72:27:17.7
04:47:41.50 +69:27:47.8
05:36:57.85 +65:42:05.7
05:51:19.03 +72:42:38.2
05:38:13.79 +68:50:54.9
04:45:29.78 +74:16:14.4
06:28:02.54 +72:19:51.9
05:44:29.09 +70:20:34.0
04:40:44.25 +69:05:34.4
04:49:42.22 +75:05:48.9
04:24:13.15 +67:07:08.2
04:30:44.57 +74:12:33.4
04:54:16.84 +65:21:23.2
03:20:24.91 +70:25:30.5
04:41:44.13 +74:34:43.8
06:14:38.82 +70:39:51.6
04:53:44.19 +74:47:25.4
05:14:05.29 +70:19:07.5
05:11:19.59 +72:08:05.9
05:33:39.65 +64:23:07.4
05:24:32.25 +69:38:25.8
03:20:56.37 +71:13:17.8
05:50:23.86 +67:00:17.6
03:42:15.16 +71:59:39.0
04:24:34.43 +69:53:54.5
04:32:13.20 +69:46:33.9
03:41:25.57 +68:24:22.9
05:07:08.88 +65:22:12.0
03:36:50.18 +72:50:03.8
03:25:13.90 +73:15:13.9
06:07:10.79 +71:30:10.3
05:36:48.01 +64:22:23.6
06:10:05.98 +69:59:13.0
04:09:14.33 +70:14:49.4
03:56:03.36 +69:57:43.5
05:22:05.63 +66:32:17.4
03:37:19.76 +67:04:59.2
03:53:39.59 +67:23:17.3
05:19:37.55 +70:19:20.9
05:18:23.35 +72:55:11.7
05:11:29.94 +74:28:23.6
03:33:02.07 +68:48:58.5
05:45:03.32 +65:00:23.3
03:25:02.01 +73:22:53.5
05:06:40.14 +64:59:44.7
04:10:48.95 +74:38:56.2
03:43:52.01 +74:14:46.5
04:18:40.06 +75:11:20.7
05:31:19.79 +67:14:13.2
05:29:51.31 +72:20:59.5
04:21:07.90 +66:11:01.9
05:13:28.28 +65:11:51.8
04:54:44.77 +65:04:13.6
03:55:47.22 +71:26:44.6
03:22:47.79 +73:32:35.9
03:53:52.72 +67:13:28.9
04:25:22.03 +65:57:39.5
05:34:52.29 +63:51:44.1
05:16:24.61 +64:47:32.3
05:35:04.26 +72:27:17.1
04:24:11.80 +67:34:12.8
04:37:49.74 +72:49:37.5
05:54:11.39 +67:01:23.8
05:56:04.67 +70:14:12.8
04:25:57.53 +74:11:24.2
05:31:24.44 +64:40:05.9
04:09:07.71 +72:38:02.6
05:19:26.63 +71:43:15.1
05:12:56.01 +64:55:32.5
03:32:37.82 +67:01:40.1
05:27:07.73 +72:06:05.0
05:16:17.22 +65:08:05.1
03:29:14.41 +73:23:38.8
04:01:43.14 +71:19:25.4
04:56:17.58 +74:56:41.9
04:31:36.79 +68:45:09.4
04:37:06.68 +72:47:26.3
05:23:14.34 +65:48:38.9
05:29:57.61 +69:11:16.2
04:24:04.82 +74:15:13.5
05:39:25.07 +64:10:37.1
05:42:20.01 +64:09:42.7
03:16:55.41 +73:53:12.4
03:45:53.23 +72:40:39.1
05:44:37.98 +73:20:10.6
05:46:48.92 +66:28:26.6
03:35:34.12 +69:25:03.1
04:30:07.39 +73:12:23.1
03:48:35.94 +69:13:56.1
04:39:44.78 +68:25:39.7
04:31:51.47 +68:47:20.7
04:48:52.85 +68:02:47.7
04:23:00.46 +74:09:13.0
05:54:03.79 +68:47:47.7
03:41:55.93 +68:36:21.3
04:17:23.80 +72:57:01.5
06:33:00.92 +72:03:24.2
03:20:23.08 +73:29:18.2
04:56:17.99 +74:32:46.5
04:36:00.66 +66:19:30.6
04:35:14.02 +73:59:21.8
03:21:28.87 +73:21:25.5
05:07:09.90 +71:01:44.5
06:07:07.49 +71:41:35.8
05:23:27.55 +69:02:17.9
05:51:06.98 +68:31:25.3
03:39:40.89 +67:26:56.5
04:53:40.39 +72:30:31.2
04:10:06.87 +69:49:16.0
06:05:13.45 +72:24:08.9
06:03:50.99 +73:04:20.1
05:39:08.59 +63:44:03.5
06:09:47.66 +70:46:43.2
06:05:30.63 +67:02:43.0
05:59:53.80 +73:38:42.1
05:53:35.29 +73:35:24.6
04:56:17.86 +70:32:23.6
04:14:31.06 +70:43:07.2
05:58:04.61 +72:58:26.4
05:28:18.47 +70:24:25.6
05:12:37.92 +64:29:47.3
05:12:13.95 +64:51:32.3
05:56:55.39 +71:35:45.3
03:54:53.76 +74:53:41.2
05:34:04.47 +64:45:42.1
05:29:38.37 +70:26:14.6
04:42:28.06 +68:36:51.9
05:16:13.49 +71:25:50.1
05:03:39.77 +71:19:17.3
05:47:40.79 +66:13:52.4
05:26:02.10 +66:01:33.7
05:34:57.16 +70:26:59.4
03:53:54.20 +71:11:43.5
04:05:44.86 +75:02:48.9
05:36:31.68 +64:13:37.6
05:07:01.17 +73:43:57.8
05:41:47.60 +64:19:31.1
04:37:00.33 +67:41:14.3
04:54:03.20 +71:36:09.4
04:55:03.40 +73:08:18.3
03:51:41.54 +72:30:41.4
03:54:25.44 +67:41:53.2
04:12:18.90 +66:10:04.5
04:56:44.03 +67:40:08.8
###################################################################################
05:25:42.43 +72:10:43.5 -- not an asteroid (will add it to exclusion list)
05:03:00.83 +71:37:27.5 -- not an asteroid (will add it to exclusion list)
05:48:21.87 +64:32:09.8 -- not an asteroid (will add it to exclusion list)
05:03:11.35 +69:43:42.8 -- not an asteroid (will add it to exclusion list)
05:03:18.16 +72:39:59.7 -- not an asteroid (will add it to exclusion list)
04:20:25.52 +74:02:55.8 -- not an asteroid (will add it to exclusion list)
04:33:03.65 +69:49:45.6 -- not an asteroid (will add it to exclusion list)
04:06:37.63 +68:36:19.4 -- not an asteroid (will add it to exclusion list)
05:25:12.41 +66:12:18.6 -- not an asteroid (will add it to exclusion list)
04:56:22.40 +72:43:26.7 -- not an asteroid (will add it to exclusion list)
04:55:22.27 +66:47:32.8 -- not an asteroid (will add it to exclusion list)
05:59:14.60 +70:12:05.1 -- not an asteroid (will add it to exclusion list)
04:49:37.46 +69:17:39.2 -- not an asteroid (will add it to exclusion list)
04:28:13.58 +68:28:43.7 -- not an asteroid (will add it to exclusion list)
05:15:55.15 +73:39:59.9 -- not an asteroid (will add it to exclusion list)
06:14:59.89 +70:38:32.0 -- not an asteroid (will add it to exclusion list)
05:01:49.26 +66:03:52.6 -- not an asteroid (will add it to exclusion list)
05:34:40.32 +67:06:25.9 -- not an asteroid (will add it to exclusion list)
04:54:19.78 +68:57:49.3 -- not an asteroid (will add it to exclusion list)
05:02:53.80 +65:01:14.0 -- not an asteroid (will add it to exclusion list)
04:32:28.63 +67:14:24.4 -- not an asteroid (will add it to exclusion list)
04:02:19.72 +70:42:08.6 -- not an asteroid (will add it to exclusion list)
05:38:34.63 +70:25:44.9 -- not an asteroid (will add it to exclusion list)
05:13:00.11 +68:41:29.0 -- not an asteroid (will add it to exclusion list)
03:24:31.89 +70:39:05.7 -- not an asteroid (will add it to exclusion list)
05:44:46.41 +64:00:07.9 -- not an asteroid (will add it to exclusion list)
05:27:07.63 +72:34:27.7 -- not an asteroid (will add it to exclusion list)
05:52:27.86 +70:32:03.8 -- not an asteroid (will add it to exclusion list)
03:45:58.83 +68:00:22.9 -- not an asteroid (will add it to exclusion list)
04:42:14.62 +69:04:10.2 -- not an asteroid (will add it to exclusion list)
04:57:37.94 +70:38:34.8 -- not an asteroid (will add it to exclusion list)
04:48:51.80 +74:27:59.9 -- not an asteroid (will add it to exclusion list)
05:32:38.74 +71:28:25.8 -- not an asteroid (will add it to exclusion list)
05:38:30.12 +74:15:31.5 -- not an asteroid (will add it to exclusion list)
05:45:07.80 +70:54:04.3 -- not an asteroid (will add it to exclusion list)
05:51:35.41 +68:00:53.7 -- not an asteroid (will add it to exclusion list)
03:37:05.47 +69:37:35.6 -- not an asteroid (will add it to exclusion list)
05:17:15.82 +73:34:58.5 -- not an asteroid (will add it to exclusion list)
05:48:53.23 +73:08:42.4 -- not an asteroid (will add it to exclusion list)
05:42:16.32 +68:55:14.9 -- not an asteroid (will add it to exclusion list)
04:03:46.01 +74:47:17.6 -- not an asteroid (will add it to exclusion list)
04:24:07.64 +66:28:21.7 -- not an asteroid (will add it to exclusion list)
04:41:23.25 +72:55:31.7 -- not an asteroid (will add it to exclusion list)
04:49:57.56 +67:08:31.1 -- not an asteroid (will add it to exclusion list)
03:34:59.11 +71:38:54.0 -- not an asteroid (will add it to exclusion list)
04:46:14.94 +66:27:36.0 -- not an asteroid (will add it to exclusion list)
03:58:46.26 +73:22:06.9 -- not an asteroid (will add it to exclusion list)
05:53:04.13 +64:13:56.7 -- not an asteroid (will add it to exclusion list)
04:29:18.98 +69:31:54.8 -- not an asteroid (will add it to exclusion list)
04:20:01.28 +68:13:24.2 -- not an asteroid (will add it to exclusion list)
04:54:50.65 +66:57:16.2 -- not an asteroid (will add it to exclusion list)
05:51:22.12 +64:43:30.3 -- not an asteroid (will add it to exclusion list)
05:02:57.10 +65:09:02.1 -- not an asteroid (will add it to exclusion list)
05:15:57.20 +70:34:25.2 -- not an asteroid (will add it to exclusion list)
06:25:10.05 +70:16:23.9 -- not an asteroid (will add it to exclusion list)
05:26:37.67 +64:37:46.4 -- not an asteroid (will add it to exclusion list)
05:36:37.21 +74:18:46.1 -- not an asteroid (will add it to exclusion list)
05:54:33.59 +72:46:27.0 -- not an asteroid (will add it to exclusion list)
05:01:18.34 +66:42:39.3 -- not an asteroid (will add it to exclusion list)
03:35:57.74 +72:27:17.7 -- not an asteroid (will add it to exclusion list)
04:47:41.50 +69:27:47.8 -- not an asteroid (will add it to exclusion list)
05:36:57.85 +65:42:05.7 -- not an asteroid (will add it to exclusion list)
05:51:19.03 +72:42:38.2 -- not an asteroid (will add it to exclusion list)
05:38:13.79 +68:50:54.9 -- not an asteroid (will add it to exclusion list)
04:45:29.78 +74:16:14.4 -- not an asteroid (will add it to exclusion list)
06:28:02.54 +72:19:51.9 -- not an asteroid (will add it to exclusion list)
05:44:29.09 +70:20:34.0 -- not an asteroid (will add it to exclusion list)
04:40:44.25 +69:05:34.4 -- not an asteroid (will add it to exclusion list)
04:49:42.22 +75:05:48.9 -- not an asteroid (will add it to exclusion list)
04:24:13.15 +67:07:08.2 -- not an asteroid (will add it to exclusion list)
04:30:44.57 +74:12:33.4 -- not an asteroid (will add it to exclusion list)
04:54:16.84 +65:21:23.2 -- not an asteroid (will add it to exclusion list)
03:20:24.91 +70:25:30.5 -- not an asteroid (will add it to exclusion list)
04:41:44.13 +74:34:43.8 -- not an asteroid (will add it to exclusion list)
06:14:38.82 +70:39:51.6 -- not an asteroid (will add it to exclusion list)
04:53:44.19 +74:47:25.4 -- not an asteroid (will add it to exclusion list)
05:14:05.29 +70:19:07.5 -- not an asteroid (will add it to exclusion list)
05:11:19.59 +72:08:05.9 -- not an asteroid (will add it to exclusion list)
05:33:39.65 +64:23:07.4 -- not an asteroid (will add it to exclusion list)
05:24:32.25 +69:38:25.8 -- not an asteroid (will add it to exclusion list)
03:20:56.37 +71:13:17.8 -- not an asteroid (will add it to exclusion list)
05:50:23.86 +67:00:17.6 -- not an asteroid (will add it to exclusion list)
03:42:15.16 +71:59:39.0 -- not an asteroid (will add it to exclusion list)
04:24:34.43 +69:53:54.5 -- not an asteroid (will add it to exclusion list)
04:32:13.20 +69:46:33.9 -- not an asteroid (will add it to exclusion list)
03:41:25.57 +68:24:22.9 -- not an asteroid (will add it to exclusion list)
05:07:08.88 +65:22:12.0 -- not an asteroid (will add it to exclusion list)
03:36:50.18 +72:50:03.8 -- not an asteroid (will add it to exclusion list)
03:25:13.90 +73:15:13.9 -- not an asteroid (will add it to exclusion list)
06:07:10.79 +71:30:10.3 -- not an asteroid (will add it to exclusion list)
05:36:48.01 +64:22:23.6 -- not an asteroid (will add it to exclusion list)
06:10:05.98 +69:59:13.0 -- not an asteroid (will add it to exclusion list)
04:09:14.33 +70:14:49.4 -- not an asteroid (will add it to exclusion list)
03:56:03.36 +69:57:43.5 -- not an asteroid (will add it to exclusion list)
05:22:05.63 +66:32:17.4 -- not an asteroid (will add it to exclusion list)
03:37:19.76 +67:04:59.2 -- not an asteroid (will add it to exclusion list)
03:53:39.59 +67:23:17.3 -- not an asteroid (will add it to exclusion list)
05:19:37.55 +70:19:20.9 -- not an asteroid (will add it to exclusion list)
05:18:23.35 +72:55:11.7 -- not an asteroid (will add it to exclusion list)
05:11:29.94 +74:28:23.6 -- not an asteroid (will add it to exclusion list)
03:33:02.07 +68:48:58.5 -- not an asteroid (will add it to exclusion list)
05:45:03.32 +65:00:23.3 -- not an asteroid (will add it to exclusion list)
03:25:02.01 +73:22:53.5 -- not an asteroid (will add it to exclusion list)
05:06:40.14 +64:59:44.7 -- not an asteroid (will add it to exclusion list)
04:10:48.95 +74:38:56.2 -- not an asteroid (will add it to exclusion list)
03:43:52.01 +74:14:46.5 -- not an asteroid (will add it to exclusion list)
04:18:40.06 +75:11:20.7 -- not an asteroid (will add it to exclusion list)
05:31:19.79 +67:14:13.2 -- not an asteroid (will add it to exclusion list)
05:29:51.31 +72:20:59.5 -- not an asteroid (will add it to exclusion list)
04:21:07.90 +66:11:01.9 -- not an asteroid (will add it to exclusion list)
05:13:28.28 +65:11:51.8 -- not an asteroid (will add it to exclusion list)
04:54:44.77 +65:04:13.6 -- not an asteroid (will add it to exclusion list)
03:55:47.22 +71:26:44.6 -- not an asteroid (will add it to exclusion list)
03:22:47.79 +73:32:35.9 -- not an asteroid (will add it to exclusion list)
03:53:52.72 +67:13:28.9 -- not an asteroid (will add it to exclusion list)
04:25:22.03 +65:57:39.5 -- not an asteroid (will add it to exclusion list)
05:34:52.29 +63:51:44.1 -- not an asteroid (will add it to exclusion list)
05:16:24.61 +64:47:32.3 -- not an asteroid (will add it to exclusion list)
05:35:04.26 +72:27:17.1 -- not an asteroid (will add it to exclusion list)
04:24:11.80 +67:34:12.8 -- not an asteroid (will add it to exclusion list)
04:37:49.74 +72:49:37.5 -- not an asteroid (will add it to exclusion list)
05:54:11.39 +67:01:23.8 -- not an asteroid (will add it to exclusion list)
05:56:04.67 +70:14:12.8 -- not an asteroid (will add it to exclusion list)
04:25:57.53 +74:11:24.2 -- not an asteroid (will add it to exclusion list)
05:31:24.44 +64:40:05.9 -- not an asteroid (will add it to exclusion list)
04:09:07.71 +72:38:02.6 -- not an asteroid (will add it to exclusion list)
05:19:26.63 +71:43:15.1 -- not an asteroid (will add it to exclusion list)
05:12:56.01 +64:55:32.5 -- not an asteroid (will add it to exclusion list)
03:32:37.82 +67:01:40.1 -- not an asteroid (will add it to exclusion list)
05:27:07.73 +72:06:05.0 -- not an asteroid (will add it to exclusion list)
05:16:17.22 +65:08:05.1 -- not an asteroid (will add it to exclusion list)
03:29:14.41 +73:23:38.8 -- not an asteroid (will add it to exclusion list)
04:01:43.14 +71:19:25.4 -- not an asteroid (will add it to exclusion list)
04:56:17.58 +74:56:41.9 -- not an asteroid (will add it to exclusion list)
04:31:36.79 +68:45:09.4 -- not an asteroid (will add it to exclusion list)
04:37:06.68 +72:47:26.3 -- not an asteroid (will add it to exclusion list)
05:23:14.34 +65:48:38.9 -- not an asteroid (will add it to exclusion list)
05:29:57.61 +69:11:16.2 -- not an asteroid (will add it to exclusion list)
04:24:04.82 +74:15:13.5 -- not an asteroid (will add it to exclusion list)
05:39:25.07 +64:10:37.1 -- not an asteroid (will add it to exclusion list)
05:42:20.01 +64:09:42.7 -- not an asteroid (will add it to exclusion list)
03:16:55.41 +73:53:12.4 -- not an asteroid (will add it to exclusion list)
03:45:53.23 +72:40:39.1 -- not an asteroid (will add it to exclusion list)
05:44:37.98 +73:20:10.6 -- not an asteroid (will add it to exclusion list)
05:46:48.92 +66:28:26.6 -- not an asteroid (will add it to exclusion list)
03:35:34.12 +69:25:03.1 -- not an asteroid (will add it to exclusion list)
04:30:07.39 +73:12:23.1 -- not an asteroid (will add it to exclusion list)
03:48:35.94 +69:13:56.1 -- not an asteroid (will add it to exclusion list)
04:39:44.78 +68:25:39.7 -- not an asteroid (will add it to exclusion list)
04:31:51.47 +68:47:20.7 -- not an asteroid (will add it to exclusion list)
04:48:52.85 +68:02:47.7 -- not an asteroid (will add it to exclusion list)
04:23:00.46 +74:09:13.0 -- not an asteroid (will add it to exclusion list)
05:54:03.79 +68:47:47.7 -- not an asteroid (will add it to exclusion list)
03:41:55.93 +68:36:21.3 -- not an asteroid (will add it to exclusion list)
04:17:23.80 +72:57:01.5 -- not an asteroid (will add it to exclusion list)
06:33:00.92 +72:03:24.2 -- not an asteroid (will add it to exclusion list)
03:20:23.08 +73:29:18.2 -- not an asteroid (will add it to exclusion list)
04:56:17.99 +74:32:46.5 -- not an asteroid (will add it to exclusion list)
04:36:00.66 +66:19:30.6 -- not an asteroid (will add it to exclusion list)
04:35:14.02 +73:59:21.8 -- not an asteroid (will add it to exclusion list)
03:21:28.87 +73:21:25.5 -- not an asteroid (will add it to exclusion list)
05:07:09.90 +71:01:44.5 -- not an asteroid (will add it to exclusion list)
06:07:07.49 +71:41:35.8 -- not an asteroid (will add it to exclusion list)
05:23:27.55 +69:02:17.9 -- not an asteroid (will add it to exclusion list)
05:51:06.98 +68:31:25.3 -- not an asteroid (will add it to exclusion list)
03:39:40.89 +67:26:56.5 -- not an asteroid (will add it to exclusion list)
04:53:40.39 +72:30:31.2 -- not an asteroid (will add it to exclusion list)
04:10:06.87 +69:49:16.0 -- not an asteroid (will add it to exclusion list)
06:05:13.45 +72:24:08.9 -- not an asteroid (will add it to exclusion list)
06:03:50.99 +73:04:20.1 -- not an asteroid (will add it to exclusion list)
05:39:08.59 +63:44:03.5 -- not an asteroid (will add it to exclusion list)
06:09:47.66 +70:46:43.2 -- not an asteroid (will add it to exclusion list)
06:05:30.63 +67:02:43.0 -- not an asteroid (will add it to exclusion list)
05:59:53.80 +73:38:42.1 -- not an asteroid (will add it to exclusion list)
05:53:35.29 +73:35:24.6 -- not an asteroid (will add it to exclusion list)
04:56:17.86 +70:32:23.6 -- not an asteroid (will add it to exclusion list)
04:14:31.06 +70:43:07.2 -- not an asteroid (will add it to exclusion list)
05:58:04.61 +72:58:26.4 -- not an asteroid (will add it to exclusion list)
05:28:18.47 +70:24:25.6 -- not an asteroid (will add it to exclusion list)
05:12:37.92 +64:29:47.3 -- not an asteroid (will add it to exclusion list)
05:12:13.95 +64:51:32.3 -- not an asteroid (will add it to exclusion list)
05:56:55.39 +71:35:45.3 -- not an asteroid (will add it to exclusion list)
03:54:53.76 +74:53:41.2 -- not an asteroid (will add it to exclusion list)
05:34:04.47 +64:45:42.1 -- not an asteroid (will add it to exclusion list)
05:29:38.37 +70:26:14.6 -- not an asteroid (will add it to exclusion list)
04:42:28.06 +68:36:51.9 -- not an asteroid (will add it to exclusion list)
05:16:13.49 +71:25:50.1 -- not an asteroid (will add it to exclusion list)
05:03:39.77 +71:19:17.3 -- not an asteroid (will add it to exclusion list)
05:47:40.79 +66:13:52.4 -- not an asteroid (will add it to exclusion list)
05:26:02.10 +66:01:33.7 -- not an asteroid (will add it to exclusion list)
05:34:57.16 +70:26:59.4 -- not an asteroid (will add it to exclusion list)
03:53:54.20 +71:11:43.5 -- not an asteroid (will add it to exclusion list)
04:05:44.86 +75:02:48.9 -- not an asteroid (will add it to exclusion list)
05:36:31.68 +64:13:37.6 -- not an asteroid (will add it to exclusion list)
05:07:01.17 +73:43:57.8 -- not an asteroid (will add it to exclusion list)
05:41:47.60 +64:19:31.1 -- not an asteroid (will add it to exclusion list)
04:37:00.33 +67:41:14.3 -- not an asteroid (will add it to exclusion list)
04:54:03.20 +71:36:09.4 -- not an asteroid (will add it to exclusion list)
04:55:03.40 +73:08:18.3 -- not an asteroid (will add it to exclusion list)
03:51:41.54 +72:30:41.4 -- not an asteroid (will add it to exclusion list)
03:54:25.44 +67:41:53.2 -- not an asteroid (will add it to exclusion list)
04:12:18.90 +66:10:04.5 -- not an asteroid (will add it to exclusion list)
04:56:44.03 +67:40:08.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
03:16:55.41 +73:53:12.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:20:23.08 +73:29:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:20:24.91 +70:25:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:20:56.37 +71:13:17.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:21:28.87 +73:21:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:22:47.79 +73:32:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:24:31.89 +70:39:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:25:02.01 +73:22:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:25:13.90 +73:15:13.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:29:14.41 +73:23:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:32:37.82 +67:01:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:33:02.07 +68:48:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:59.11 +71:38:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:34.12 +69:25:03.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:57.74 +72:27:17.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:50.18 +72:50:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:05.47 +69:37:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:19.76 +67:04:59.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:39:40.89 +67:26:56.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:25.57 +68:24:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:55.93 +68:36:21.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:42:15.16 +71:59:39.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:52.01 +74:14:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:53.23 +72:40:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:58.83 +68:00:22.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:35.94 +69:13:56.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:41.54 +72:30:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:39.59 +67:23:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:52.72 +67:13:28.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:54.20 +71:11:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:25.44 +67:41:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:54:53.76 +74:53:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:55:47.22 +71:26:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:56:03.36 +69:57:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:58:46.26 +73:22:06.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:01:43.14 +71:19:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:02:19.72 +70:42:08.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:03:46.01 +74:47:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:44.86 +75:02:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:06:37.63 +68:36:19.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:09:07.71 +72:38:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:09:14.33 +70:14:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:10:06.87 +69:49:16.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:10:48.95 +74:38:56.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:12:18.90 +66:10:04.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:14:31.06 +70:43:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:17:23.80 +72:57:01.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:18:40.06 +75:11:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:20:01.28 +68:13:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:20:25.52 +74:02:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:21:07.90 +66:11:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:23:00.46 +74:09:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:04.82 +74:15:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:07.64 +66:28:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:11.80 +67:34:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:13.15 +67:07:08.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:34.43 +69:53:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:22.03 +65:57:39.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:57.53 +74:11:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:28:13.58 +68:28:43.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:29:18.98 +69:31:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:30:07.39 +73:12:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:30:44.57 +74:12:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:31:36.79 +68:45:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:31:51.47 +68:47:20.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:13.20 +69:46:33.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:28.63 +67:14:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:33:03.65 +69:49:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:14.02 +73:59:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:00.66 +66:19:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:00.33 +67:41:14.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:06.68 +72:47:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:37:49.74 +72:49:37.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:39:44.78 +68:25:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:40:44.25 +69:05:34.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:41:23.25 +72:55:31.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:41:44.13 +74:34:43.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:42:14.62 +69:04:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:42:28.06 +68:36:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:45:29.78 +74:16:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:46:14.94 +66:27:36.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:47:41.50 +69:27:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:48:51.80 +74:27:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:48:52.85 +68:02:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:49:37.46 +69:17:39.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:49:42.22 +75:05:48.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:49:57.56 +67:08:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:40.39 +72:30:31.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:53:44.19 +74:47:25.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:03.20 +71:36:09.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:16.84 +65:21:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:19.78 +68:57:49.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:44.77 +65:04:13.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:50.65 +66:57:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:03.40 +73:08:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:22.27 +66:47:32.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:17.58 +74:56:41.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:17.86 +70:32:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:17.99 +74:32:46.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:22.40 +72:43:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:44.03 +67:40:08.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:37.94 +70:38:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:18.34 +66:42:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:49.26 +66:03:52.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:53.80 +65:01:14.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:57.10 +65:09:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:00.83 +71:37:27.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:11.35 +69:43:42.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:18.16 +72:39:59.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:39.77 +71:19:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:40.14 +64:59:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:01.17 +73:43:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:08.88 +65:22:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:09.90 +71:01:44.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:11:19.59 +72:08:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:11:29.94 +74:28:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:12:13.95 +64:51:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:12:37.92 +64:29:47.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:12:56.01 +64:55:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:13:00.11 +68:41:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:13:28.28 +65:11:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:14:05.29 +70:19:07.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:55.15 +73:39:59.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:57.20 +70:34:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:13.49 +71:25:50.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:17.22 +65:08:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:24.61 +64:47:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:15.82 +73:34:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:18:23.35 +72:55:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:26.63 +71:43:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:37.55 +70:19:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:05.63 +66:32:17.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:14.34 +65:48:38.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:23:27.55 +69:02:17.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:32.25 +69:38:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:12.41 +66:12:18.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:42.43 +72:10:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:02.10 +66:01:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:26:37.67 +64:37:46.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:07.63 +72:34:27.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:07.73 +72:06:05.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:28:18.47 +70:24:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:38.37 +70:26:14.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:51.31 +72:20:59.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:57.61 +69:11:16.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:19.79 +67:14:13.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:24.44 +64:40:05.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:32:38.74 +71:28:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:39.65 +64:23:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:04.47 +64:45:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:40.32 +67:06:25.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:52.29 +63:51:44.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:34:57.16 +70:26:59.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:35:04.26 +72:27:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:31.68 +64:13:37.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:37.21 +74:18:46.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:48.01 +64:22:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:57.85 +65:42:05.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:13.79 +68:50:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:30.12 +74:15:31.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:38:34.63 +70:25:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:08.59 +63:44:03.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:25.07 +64:10:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:47.60 +64:19:31.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:16.32 +68:55:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:42:20.01 +64:09:42.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:29.09 +70:20:34.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:37.98 +73:20:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:46.41 +64:00:07.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:03.32 +65:00:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:07.80 +70:54:04.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:48.92 +66:28:26.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:47:40.79 +66:13:52.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:21.87 +64:32:09.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:53.23 +73:08:42.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:50:23.86 +67:00:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:06.98 +68:31:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:19.03 +72:42:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:22.12 +64:43:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:51:35.41 +68:00:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:52:27.86 +70:32:03.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:04.13 +64:13:56.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:35.29 +73:35:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:03.79 +68:47:47.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:11.39 +67:01:23.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:33.59 +72:46:27.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:04.67 +70:14:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:56:55.39 +71:35:45.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:04.61 +72:58:26.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:14.60 +70:12:05.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:53.80 +73:38:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:50.99 +73:04:20.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:13.45 +72:24:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:30.63 +67:02:43.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:07.49 +71:41:35.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:10.79 +71:30:10.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:47.66 +70:46:43.2 -- does not seem to be a hot pixel (will add it to exclusion list)
06:10:05.98 +69:59:13.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:38.82 +70:39:51.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:14:59.89 +70:38:32.0 -- does not seem to be a hot pixel (will add it to exclusion list)
06:25:10.05 +70:16:23.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:28:02.54 +72:19:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:33:00.92 +72:03:24.2 -- 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)
03:16:55.41 +73:53:12.4 -- not a known variable star
03:20:23.08 +73:29:18.2 -- not a known variable star
03:20:24.91 +70:25:30.5 -- not a known variable star
03:20:56.37 +71:13:17.8 -- not a known variable star
03:21:28.87 +73:21:25.5 -- not a known variable star
03:22:47.79 +73:32:35.9 -- not a known variable star
03:24:31.89 +70:39:05.7 -- not a known variable star
03:25:02.01 +73:22:53.5 -- not a known variable star
03:25:13.90 +73:15:13.9 -- a known variable star
03:29:14.41 +73:23:38.8 -- not a known variable star
03:32:37.82 +67:01:40.1 -- not a known variable star
03:33:02.07 +68:48:58.5 -- not a known variable star
03:34:59.11 +71:38:54.0 -- a known variable star
03:35:34.12 +69:25:03.1 -- not a known variable star
03:35:57.74 +72:27:17.7 -- not a known variable star
03:36:50.18 +72:50:03.8 -- not a known variable star
03:37:05.47 +69:37:35.6 -- not a known variable star
03:37:19.76 +67:04:59.2 -- not a known variable star
03:39:40.89 +67:26:56.5 -- not a known variable star
03:41:25.57 +68:24:22.9 -- not a known variable star
03:41:55.93 +68:36:21.3 -- not a known variable star
03:42:15.16 +71:59:39.0 -- not a known variable star
03:43:52.01 +74:14:46.5 -- not a known variable star
03:45:53.23 +72:40:39.1 -- not a known variable star
03:45:58.83 +68:00:22.9 -- not a known variable star
03:48:35.94 +69:13:56.1 -- not a known variable star
03:51:41.54 +72:30:41.4 -- not a known variable star
03:53:39.59 +67:23:17.3 -- not a known variable star
03:53:52.72 +67:13:28.9 -- not a known variable star
03:53:54.20 +71:11:43.5 -- not a known variable star
03:54:25.44 +67:41:53.2 -- not a known variable star
03:54:53.76 +74:53:41.2 -- not a known variable star
03:55:47.22 +71:26:44.6 -- not a known variable star
03:56:03.36 +69:57:43.5 -- not a known variable star
03:58:46.26 +73:22:06.9 -- not a known variable star
04:01:43.14 +71:19:25.4 -- a known variable star
04:02:19.72 +70:42:08.6 -- not a known variable star
04:03:46.01 +74:47:17.6 -- not a known variable star
04:05:44.86 +75:02:48.9 -- not a known variable star
04:06:37.63 +68:36:19.4 -- not a known variable star
04:09:07.71 +72:38:02.6 -- not a known variable star
04:09:14.33 +70:14:49.4 -- not a known variable star
04:10:06.87 +69:49:16.0 -- not a known variable star
04:10:48.95 +74:38:56.2 -- not a known variable star
04:12:18.90 +66:10:04.5 -- not a known variable star
04:14:31.06 +70:43:07.2 -- not a known variable star
04:17:23.80 +72:57:01.5 -- not a known variable star
04:18:40.06 +75:11:20.7 -- not a known variable star
04:20:01.28 +68:13:24.2 -- not a known variable star
04:20:25.52 +74:02:55.8 -- not a known variable star
04:21:07.90 +66:11:01.9 -- not a known variable star
04:23:00.46 +74:09:13.0 -- not a known variable star
04:24:04.82 +74:15:13.5 -- not a known variable star
04:24:07.64 +66:28:21.7 -- not a known variable star
04:24:11.80 +67:34:12.8 -- not a known variable star
04:24:13.15 +67:07:08.2 -- not a known variable star
04:24:34.43 +69:53:54.5 -- not a known variable star
04:25:22.03 +65:57:39.5 -- not a known variable star
04:25:57.53 +74:11:24.2 -- a known variable star
04:28:13.58 +68:28:43.7 -- not a known variable star
04:29:18.98 +69:31:54.8 -- not a known variable star
04:30:07.39 +73:12:23.1 -- not a known variable star
04:30:44.57 +74:12:33.4 -- not a known variable star
04:31:36.79 +68:45:09.4 -- not a known variable star
04:31:51.47 +68:47:20.7 -- not a known variable star
04:32:13.20 +69:46:33.9 -- not a known variable star
04:32:28.63 +67:14:24.4 -- not a known variable star
04:33:03.65 +69:49:45.6 -- not a known variable star
04:35:14.02 +73:59:21.8 -- not a known variable star
04:36:00.66 +66:19:30.6 -- not a known variable star
04:37:00.33 +67:41:14.3 -- a known variable star
04:37:06.68 +72:47:26.3 -- not a known variable star
04:37:49.74 +72:49:37.5 -- not a known variable star
04:39:44.78 +68:25:39.7 -- not a known variable star
04:40:44.25 +69:05:34.4 -- a known variable star
04:41:23.25 +72:55:31.7 -- not a known variable star
04:41:44.13 +74:34:43.8 -- not a known variable star
04:42:14.62 +69:04:10.2 -- not a known variable star
04:42:28.06 +68:36:51.9 -- not a known variable star
04:45:29.78 +74:16:14.4 -- not a known variable star
04:46:14.94 +66:27:36.0 -- not a known variable star
04:47:41.50 +69:27:47.8 -- a known variable star
04:48:51.80 +74:27:59.9 -- not a known variable star
04:48:52.85 +68:02:47.7 -- not a known variable star
04:49:37.46 +69:17:39.2 -- not a known variable star
04:49:42.22 +75:05:48.9 -- not a known variable star
04:49:57.56 +67:08:31.1 -- a known variable star
04:53:40.39 +72:30:31.2 -- not a known variable star
04:53:44.19 +74:47:25.4 -- a known variable star
04:54:03.20 +71:36:09.4 -- not a known variable star
04:54:16.84 +65:21:23.2 -- not a known variable star
04:54:19.78 +68:57:49.3 -- a known variable star
04:54:44.77 +65:04:13.6 -- a known variable star
04:54:50.65 +66:57:16.2 -- not a known variable star
04:55:03.40 +73:08:18.3 -- not a known variable star
04:55:22.27 +66:47:32.8 -- not a known variable star
04:56:17.58 +74:56:41.9 -- not a known variable star
04:56:17.86 +70:32:23.6 -- not a known variable star
04:56:17.99 +74:32:46.5 -- not a known variable star
04:56:22.40 +72:43:26.7 -- not a known variable star
04:56:44.03 +67:40:08.8 -- a known variable star
04:57:37.94 +70:38:34.8 -- not a known variable star
05:01:18.34 +66:42:39.3 -- not a known variable star
05:01:49.26 +66:03:52.6 -- not a known variable star
05:02:53.80 +65:01:14.0 -- not a known variable star
05:02:57.10 +65:09:02.1 -- not a known variable star
05:03:00.83 +71:37:27.5 -- not a known variable star
05:03:11.35 +69:43:42.8 -- not a known variable star
05:03:18.16 +72:39:59.7 -- not a known variable star
05:03:39.77 +71:19:17.3 -- not a known variable star
05:06:40.14 +64:59:44.7 -- not a known variable star
05:07:01.17 +73:43:57.8 -- not a known variable star
05:07:08.88 +65:22:12.0 -- a known variable star
05:07:09.90 +71:01:44.5 -- not a known variable star
05:11:19.59 +72:08:05.9 -- not a known variable star
05:11:29.94 +74:28:23.6 -- not a known variable star
05:12:13.95 +64:51:32.3 -- not a known variable star
05:12:37.92 +64:29:47.3 -- not a known variable star
05:12:56.01 +64:55:32.5 -- not a known variable star
05:13:00.11 +68:41:29.0 -- not a known variable star
05:13:28.28 +65:11:51.8 -- not a known variable star
05:14:05.29 +70:19:07.5 -- not a known variable star
05:15:55.15 +73:39:59.9 -- not a known variable star
05:15:57.20 +70:34:25.2 -- a known variable star
05:16:13.49 +71:25:50.1 -- not a known variable star
05:16:17.22 +65:08:05.1 -- not a known variable star
05:16:24.61 +64:47:32.3 -- not a known variable star
05:17:15.82 +73:34:58.5 -- not a known variable star
05:18:23.35 +72:55:11.7 -- not a known variable star
05:19:26.63 +71:43:15.1 -- not a known variable star
05:19:37.55 +70:19:20.9 -- not a known variable star
05:22:05.63 +66:32:17.4 -- not a known variable star
05:23:14.34 +65:48:38.9 -- not a known variable star
05:23:27.55 +69:02:17.9 -- not a known variable star
05:24:32.25 +69:38:25.8 -- not a known variable star
05:25:12.41 +66:12:18.6 -- not a known variable star
05:25:42.43 +72:10:43.5 -- a known variable star
05:26:02.10 +66:01:33.7 -- not a known variable star
05:26:37.67 +64:37:46.4 -- not a known variable star
05:27:07.63 +72:34:27.7 -- a known variable star
05:27:07.73 +72:06:05.0 -- not a known variable star
05:28:18.47 +70:24:25.6 -- not a known variable star
05:29:38.37 +70:26:14.6 -- not a known variable star
05:29:51.31 +72:20:59.5 -- not a known variable star
05:29:57.61 +69:11:16.2 -- not a known variable star
05:31:19.79 +67:14:13.2 -- not a known variable star
05:31:24.44 +64:40:05.9 -- not a known variable star
05:32:38.74 +71:28:25.8 -- not a known variable star
05:33:39.65 +64:23:07.4 -- a known variable star
05:34:04.47 +64:45:42.1 -- not a known variable star
05:34:40.32 +67:06:25.9 -- not a known variable star
05:34:52.29 +63:51:44.1 -- not a known variable star
05:34:57.16 +70:26:59.4 -- not a known variable star
05:35:04.26 +72:27:17.1 -- not a known variable star
05:36:31.68 +64:13:37.6 -- not a known variable star
05:36:37.21 +74:18:46.1 -- not a known variable star
05:36:48.01 +64:22:23.6 -- not a known variable star
05:36:57.85 +65:42:05.7 -- not a known variable star
05:38:13.79 +68:50:54.9 -- not a known variable star
05:38:30.12 +74:15:31.5 -- not a known variable star
05:38:34.63 +70:25:44.9 -- a known variable star
05:39:08.59 +63:44:03.5 -- not a known variable star
05:39:25.07 +64:10:37.1 -- not a known variable star
05:41:47.60 +64:19:31.1 -- a known variable star
05:42:16.32 +68:55:14.9 -- not a known variable star
05:42:20.01 +64:09:42.7 -- not a known variable star
05:44:29.09 +70:20:34.0 -- not a known variable star
05:44:37.98 +73:20:10.6 -- not a known variable star
05:44:46.41 +64:00:07.9 -- not a known variable star
05:45:03.32 +65:00:23.3 -- not a known variable star
05:45:07.80 +70:54:04.3 -- not a known variable star
05:46:48.92 +66:28:26.6 -- a known variable star
05:47:40.79 +66:13:52.4 -- not a known variable star
05:48:21.87 +64:32:09.8 -- not a known variable star
05:48:53.23 +73:08:42.4 -- not a known variable star
05:50:23.86 +67:00:17.6 -- not a known variable star
05:51:06.98 +68:31:25.3 -- not a known variable star
05:51:19.03 +72:42:38.2 -- not a known variable star
05:51:22.12 +64:43:30.3 -- a known variable star
05:51:35.41 +68:00:53.7 -- not a known variable star
05:52:27.86 +70:32:03.8 -- not a known variable star
05:53:04.13 +64:13:56.7 -- not a known variable star
05:53:35.29 +73:35:24.6 -- not a known variable star
05:54:03.79 +68:47:47.7 -- not a known variable star
05:54:11.39 +67:01:23.8 -- not a known variable star
05:54:33.59 +72:46:27.0 -- not a known variable star
05:56:04.67 +70:14:12.8 -- not a known variable star
05:56:55.39 +71:35:45.3 -- not a known variable star
05:58:04.61 +72:58:26.4 -- not a known variable star
05:59:14.60 +70:12:05.1 -- not a known variable star
05:59:53.80 +73:38:42.1 -- not a known variable star
06:03:50.99 +73:04:20.1 -- not a known variable star
06:05:13.45 +72:24:08.9 -- not a known variable star
06:05:30.63 +67:02:43.0 -- not a known variable star
06:07:07.49 +71:41:35.8 -- not a known variable star
06:07:10.79 +71:30:10.3 -- not a known variable star
06:09:47.66 +70:46:43.2 -- not a known variable star
06:10:05.98 +69:59:13.0 -- a known variable star
06:14:38.82 +70:39:51.6 -- not a known variable star
06:14:59.89 +70:38:32.0 -- not a known variable star
06:25:10.05 +70:16:23.9 -- not a known variable star
06:28:02.54 +72:19:51.9 -- a known variable star
06:33:00.92 +72:03:24.2 -- not a known variable star
Found 180 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
203 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 203 (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)2461083.79377507 -observatory 500
22:42:07.00 -08:45:59.0 Mercury (-1.1mag)
22:17:59.78 -12:08:17.3 Venus (-3.9mag)
21:12:03.56 -17:17:43.7 Mars (1.1mag)
07:09:04.41 +22:48:44.7 Jupiter (-2.6mag)
00:01:23.45 -02:11:41.4 Saturn (1.0mag)
03:39:31.41 +19:19:59.0 Uranus (5.7mag)
00:02:29.13 -01:09:35.0 Neptune (7.8mag)
20:27:51.83 -23:02:35.9 Pluto (14.6mag)
17:29:33.13 -28:20:50.4 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 362 Feb 12 01:08 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461083.79377507:
07:09:02.04 +22:48:45.6 Io (5.3mag)
07:09:13.66 +22:48:22.4 Europa (5.5mag)
07:08:54.11 +22:48:56.2 Ganymede (4.9mag)
07:09:07.56 +22:48:25.8 Callisto (6.0mag)
07:11:21.25 +23:09:03.4 Himalia (15.0mag)
07:09:04.54 +22:48:41.9 Thebe (15.8mag)
07:10:58.66 +23:11:48.6 Elara (17.0mag)
07:04:10.38 +24:01:49.3 Pasiphae (17.0mag)
07:18:05.49 +22:33:38.7 Carme (18.0mag)
00:01:18.70 -02:11:21.4 Titan (8.7mag)
00:01:24.83 -02:11:37.9 Rhea (10.1mag)
00:00:58.64 -02:13:24.9 Iapetus (11.5mag)
00:01:26.17 -02:11:27.2 Hyperion (14.7mag)
00:03:29.38 -01:58:16.7 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 12 01:08 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461083.79377507:
07:40:30.43 +22:57:17.6 JWST
16:51:43.10 +45:38:17.6 Chandra
16:39:18.40 -50:36:55.3 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 12 01:08 spacecraft.txt
############################################################
Positions of bright comets (listed at http://astro.vanbuitenen.nl/comets and http://aerith.net/comet/weekly/current.html ) from JPL HORIZONS for JD(UT)2461083.79377507 at 500
16:40:42.52 -10:51:19.0 17.7mag 10P/Tempel
03:28:56.39 +28:25:59.3 18.1mag 123P/West-Hartley
20:48:05.08 -10:09:52.5 22.4mag 141P/Machholz
00:59:38.76 +09:05:12.2 17.6mag 145P/Shoemaker-Levy 5
11:11:59.38 +29:17:29.4 17.8mag 164P/Christensen
09:38:46.43 -34:07:45.6 18.0mag 195P/Hill
15:51:00.85 -07:25:29.9 18.5mag 210P/Christensen
17:30:22.96 -21:38:28.1 17.4mag 218P/LINEAR
16:03:58.31 -18:17:30.2 15.2mag 235P/LINEAR
03:43:22.79 +25:51:19.1 17.5mag 240P/NEAT
15:02:50.54 +07:30:16.1 14.6mag 24P/Schaumasse
23:54:17.84 +04:18:49.5 18.1mag 261P/Larson
11:27:15.63 -03:35:45.4 17.4mag 29P/Schwassmann-Wachmann 1
01:07:14.10 +01:25:53.7 18.9mag 302P/Lemmon-PanSTARRS
07:06:38.54 +27:17:13.3 19.7mag 407P/PanSTARRS-Fuls
16:49:51.41 -11:18:39.8 17.5mag 40P/Vaisala 1
11:08:09.92 -09:15:55.5 16.6mag 43P/Wolf-Harrington
13:22:49.75 -05:08:01.8 19.4mag 489P/Denning
04:28:03.11 +49:24:37.7 17.7mag 493P/2024 Q2 (LONEOS)
06:02:39.68 +49:17:32.0 17.8mag 63P/Wild 1
22:55:12.00 -03:53:18.7 16.3mag 78P/Gehrels 2
19:24:25.70 -23:28:47.7 15.1mag 88P/Howell
15:22:03.91 -28:10:47.1 18.7mag P/2023 S1 (PanSTARRS)
04:43:15.36 -73:09:07.3 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:31:40.04 +31:11:08.7 18.1mag C/2017 K2 (PanSTARRS)
20:00:49.56 -64:56:16.9 18.1mag C/2020 V2 (ZTF)
17:17:06.31 +03:21:56.4 16.3mag C/2021 G2 (ATLAS)
22:45:48.62 +28:36:42.0 16.8mag C/2022 E2 (ATLAS)
03:28:20.52 +24:26:35.4 15.7mag C/2022 N2 (PANSTARRS)
09:11:51.28 +28:57:38.3 15.3mag C/2022 QE78 (ATLAS)
08:38:55.62 -07:44:22.1 16.6mag C/2022 R6 (PanSTARRS)
23:40:44.10 +48:06:39.5 17.9mag C/2023 C2 (ATLAS)
10:02:09.19 -22:05:26.3 17.5mag C/2023 F3 (ATLAS)
20:14:05.18 +61:17:15.2 17.2mag C/2023 H5 (Lemmon)
19:32:55.39 -03:17:45.2 16.1mag C/2023 R1 (PANSTARRS)
02:45:57.69 +35:47:09.9 18.5mag C/2023 RS61 (PanSTARRS)
20:43:35.86 +81:15:33.2 18.0mag C/2023 X2 (Lemmon)
06:55:25.17 +63:25:30.3 17.2mag C/2024 A1 (ATLAS)
00:31:02.36 -36:50:23.1 10.8mag C/2024 E1 (Wierzchos)
11:52:22.21 -04:22:28.6 18.1mag C/2024 G2 (ATLAS)
19:18:37.51 +00:21:19.0 19.0mag C/2024 G4 (PanSTARRS)
16:36:58.98 -02:56:27.1 17.8mag C/2024 G6 (ATLAS)
19:46:29.89 +01:31:23.3 15.7mag C/2024 J3 (ATLAS)
02:42:31.60 -33:26:45.6 15.4mag C/2024 T5 (ATLAS)
16:46:19.82 -54:22:05.7 15.3mag C/2025 A6 (Lemmon)
04:55:11.53 +66:13:06.9 16.7mag C/2025 J1 (Borisov)
00:00:00.00 +00:00:00.0 cannot get JPL HORIZONS ephemerides for non-periodic comet C/2025 K1 (ATLAS)
16:01:09.63 -20:10:15.7 15.0mag C/2025 L1 (ATLAS)
02:12:42.01 -17:37:33.6 16.7mag C/2025 Q3 (ATLAS)
01:56:56.54 +16:19:37.5 20.8mag C/2025 R2 (SWAN)
22:17:27.19 +17:32:37.1 16.8mag C/2025 R3 (PANSTARRS)
21:35:15.18 -14:41:24.7 20.4mag C/2025 T1 (ATLAS)
03:31:00.68 -25:07:50.6 17.4mag C/2026 A1 (MAPS)
20:25:58.91 +16:16:07.8 16.6mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.7K Feb 12 01:09 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
18:16:39.86 -19:51:57.30 TCP J06282145-1950371 2026-02-9.38 15.25
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
09:27:23.49 -32:00:30.90 SN 2023kuy 2026-01-21.16 15.43
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.72 -74:35:50.10 AT2026ahr 2026-01-20.19 17.09
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:24.99 +04:00:02.20 SN 2026kc 2026-01-18.61 16.1
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
14:46:54.08 -64:04:30.10 ASASSN-26ah 2026-01-15.07 16.84
23:02:43.24 +20:04:53.00 SN2025ajvh 2026-01-15.07 16.03
14:12:27.38 -30:12:29.10 ASASSN-26ag 2026-01-14.27 15.35
14:33:53.58 +05:27:35.40 SN 2025ajnc 2026-01-14.32 15.79
01:43:00.31 -34:11:40.60 AT2025afcm 2026-01-13.08 0.45
00:26:17.71 -52:11:38.60 AT2025ahal 2026-01-11.06 17.57
00:51:36.17 +29:42:40.10 SN2025ahxd 2026-01-11.21 15
10:19:19.14 -37:54:58.30 AT2025ahrt 2026-01-10.26 -0.54
14:37:48.78 +15:51:04.20 SN2025ajng 2026-01-9.42 16.35
05:01:03.70 -08:34:13.20 SN2026A 2026-01-9.28 16.83
00:02:52.11 +13:05:42.90 SN2025ajvg 2026-01-9.13 15.89
08:37:09.62 -02:18:08.80 SN2025aigm 2026-01-9.55 17.66
09:52:50.71 +39:36:55.70 SN2025ahyt 2026-01-9.37 16.97
11:22:19.08 -27:21:40.90 AT2026ta 2026-01-9.32 15.88
14:35:00.21 +00:59:11.40 SN 2025ahsa 2026-01-8.35 -2
09:25:42.42 +22:20:06.10 SN2025ahkt 2026-01-8.03 15.88
22:39:53.44 +34:53:50.00 SN 2025aikz 2026-01-7.09 16.3
08:21:20.95 +20:52:01.60 SN 2025aiks 2026-01-7.13 15.82
07:35:31.38 +09:10:32.40 AT2025ajvk 2026-01-7.12 -1.82
02:50:07.71 -16:37:02.30 AT2026nl 2026-01-7.16 14.19
14:05:12.75 -33:46:00.80 SN 2025ajmj 2026-01-7.31 14.93
12:35:08.33 +28:03:22.70 SN 2025aiaj 2026-01-5.44 15.76
05:30:00.47 -66:43:29.40 ASASSN-26af 2026-01-5.12 14.38
14:05:05.13 -44:14:24.00 ASASSN-26ac 2026-01-5.3 16.01
11:29:16.57 +20:35:09.00 AT2025alco 2026-01-4.39 15.93
16:42:59.28 +26:21:02.80 ASASSN-26ae 2026-01-4.52 14.31
04:13:46.60 -05:02:16.60 ASASSN-26ad 2026-01-4.32 14.58
05:00:01.32 -57:14:29.70 ASASSN-25fj/ASASSN-26ab 2026-01-1.19 13.38
13:53:51.35 -17:55:38.10 ASASSN-25fg 2025-12-23.33 16.66
06:18:15.27 +15:47:38.10 AT2025ahtd 2025-12-23.31 16.96
07:20:53.12 -33:02:58.20 SN 2025agvw 2025-12-23.32 16.84
02:58:15.63 +44:47:45.80 ASASSN-25fh 2025-12-23.13 15.63
04:51:03.78 -36:13:59.00 AT2025aftm 2025-12-20.14 17.35
03:12:59.31 +17:41:45.20 SN2025afzm 2025-12-20.15 17.22
13:33:14.27 -46:03:33.90 ASASSN-25fc 2025-12-19.32 SDSS
07:07:30.84 +24:37:55.60 SN2025agie 2025-12-19.19 16.96
12:31:24.34 -59:07:09.00 ASASSN-25fd 2025-12-19.06 14.94
14:02:20.59 -20:28:28.70 ASASSN-25fe 2025-12-19.34 SDSS
08:08:51.65 -16:39:31.50 ASASSN-25ff 2025-12-19.22 SDSS
00:34:05.69 +05:21:07.50 SN2025afty 2025-12-18.21 16.92
01:35:25.55 -05:40:42.00 AT2025agsf 2025-12-18.12 17.67
06:12:00.84 -46:50:40.70 AT2025aetd 2025-12-15.08 17.32
11:07:12.05 -55:12:59.00 ASASSN-25fa 2025-12-14.25 16.07
02:48:09.78 +37:45:17.90 AT2025afje 2025-12-13.28 17.65
08:17:38.99 +59:57:25.90 SN2025afcy 2025-12-13.43 16.8
22:58:25.70 +26:38:19.80 SN 2025afve 2025-12-12.1 16.63
03:44:52.10 -59:08:22.80 SN 2025aegk 2025-12-12.1 SDSS
04:55:47.45 -18:56:49.70 SN 2025aetg 2025-12-11.36 16.92
23:15:07.77 +13:10:19.80 SN 2025afwb 2025-12-11.2 17.13
02:19:39.33 -45:39:00.60 SN 2025aeqg 2025-12-10.07 16.77
02:03:03.89 +04:14:37.30 SN2025afih 2025-12-8.1 16.49
22:23:03.49 -56:35:57.50 AT2025aeei 2025-12-8.03 16.01
07:40:22.22 -10:00:59.30 AT2025aftz 2025-12-8.46 15.46
18:44:55.93 +47:57:37.60 ASASSN-25ez 2025-12-3.07 15.16
22:41:03.48 +38:58:01.90 ASASSN-25ey 2025-11-26.08 15.68
05:50:46.62 +58:54:53.50 SN 2025aedz 2025-11-24.25 16.66
06:35:50.19 -71:30:42.00 SN 2025adwn 2025-11-24.11 17.58
02:21:35.59 -14:18:04.90 AT2025aeft 2025-11-23.13 16.82
01:42:47.75 +12:31:45.10 AT2025aduf 2025-11-23.15 17.49
-rw-r--r-- 1 apache apache 6.2K Feb 12 01:08 asassn_transients_list.txt
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Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
00:42:28.44 +41:18:24.5 TCP J00422844+4118245 2025-12-22.8736 18.5mag
16:42:59.22 +26:21:02.0 TCP J16425922+2621020 2025-12-26.8538 13.0mag
08:08:08.72 -19:48:46.5 TCP J08080872-1948465 2025-12-27.7904 16.66Cmag
00:42:58.48 +41:08:11.4 PNV J00425848+4108114 2025-12-28.7654 18.9mag
07:35:31.47 +09:10:34.1 TCP J07353147+0910341 2025-12-29.7527 14.77Cmag
14:45:58.45 +39:05:10.3 TCP J14455845+3905103 2025-12-30.8196 14.1mag
00:43:23.44 +41:24:35.7 PNV J00432344+4124357 2025-12-11.684 19.7mag
00:41:01.11 +41:59:28.2 PNV J00410111+4159282 2026-01-06.1994 18.7mag
00:42:52.01 +41:14:29.2 PNV J00425201+4114292 2026-01-08.7863 18.37Cmag
02:50:07.72 -16:37:02.3 TCP J02500772-1637023 2026-01-06.6352 14.53Cmag
00:42:58.52 +41:14:44.2 PNV J00425852+4114442 2026-01-13.4991 16.89Cmag
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
-rw-r--r-- 1 apache apache 186K Feb 12 01:08 tocp_transients_list.txt
