This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.56 04:59:41.46 +67:23:00.4
143.53574 15.10405 galactic Cam Second-epoch detections are separated by 0.6" 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 | 04:59:41.46 +67:23:00.4 (user input) | T | P | (position from user input) J-Ks=0.367+/-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,2461119.6472,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:59:41.46 +67:23:00.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.79 05:05:09.09 +66:23:19.0
144.69779 14.97256 galactic Cam Second-epoch detections are separated by 2.3" 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 | 05:05:09.09 +66:23:19.0 (user input) | T | P | (position from user input) J-Ks=0.436+/-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,2461119.6472,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:05:09.09 +66:23:19.0 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.65 04:49:03.90 +69:07:43.6
141.47512 15.34864 galactic Cam Second-epoch detections are separated by 2.2" 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 | 04:49:03.90 +69:07:43.6 (user input) | T | P | (position from user input) J-Ks=0.521+/-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,2461119.6472,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:03.90 +69:07:43.6 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:51.50 +65:22:30.5 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.46 05:02:11.36 +66:07:00.4
144.75217 14.57249 galactic Cam Second-epoch detections are separated by 2.1" 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 | 05:02:11.36 +66:07:00.4 (user input) | T | P | (position from user input) J-Ks=0.510+/-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,2461119.6472,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:02:11.36 +66:07:00.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.41 05:03:35.97 +68:40:13.4
142.65702 16.14022 galactic Cam Second-epoch detections are separated by 2.0" 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 | 05:03:35.97 +68:40:13.4 (user input) | T | P | (position from user input) J-Ks=0.700+/-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,2461119.6472,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:35.97 +68:40:13.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.43 05:55:54.35 +66:08:23.3
147.51996 19.30722 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 | target | 05:55:54.35 +66:08:23.3 (user input) | T | P | (position from user input) J-Ks=0.357+/-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,2461119.6472,13.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:54.35 +66:08:23.3 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.45 05:11:38.57 +64:54:35.6
146.35300 14.70075 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 | 05:11:38.57 +64:54:35.6 (user input) | T | P | (position from user input) J-Ks=0.445+/-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,2461119.6472,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:11:38.57 +64:54:35.6 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.42 05:11:48.71 +66:41:11.0
144.82324 15.68915 galactic Cam Second-epoch detections are separated by 0.7" 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 | 05:11:48.71 +66:41:11.0 (user input) | T | P | (position from user input) J-Ks=0.581+/-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,2461119.6472,13.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:11:48.71 +66:41:11.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.44 05:25:12.19 +66:12:19.7
145.97991 16.57568 galactic Cam Second-epoch detections are separated by 2.0" 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 | 05:25:12.19 +66:12:19.7 (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,2461119.6472,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:25:12.19 +66:12:19.7 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.37 03:56:03.26 +69:57:42.2
137.59647 12.54071 galactic Cam Second-epoch detections are separated by 1.9" 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 | 03:56:03.26 +69:57:42.2 (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,2461119.6472,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:03.26 +69:57:42.2 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:13.44 +70:35:39.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.27 04:30:36.89 +74:25:32.2
136.23396 17.54663 galactic Cam Second-epoch detections are separated by 0.5" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:30:36.89 +74:25:32.2 (user input) | T | P | (position from user input) J-Ks=0.296+/-0.041 (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,2461119.6472,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:30:36.89 +74:25:32.2 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.31 06:03:51.51 +70:17:17.6
143.71698 21.55481 galactic Cam Second-epoch detections are separated by 1.9" 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 | 06:03:51.51 +70:17:17.6 (user input) | T | P | (position from user input) J-Ks=0.524+/-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,2461119.6472,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:03:51.51 +70:17:17.6 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 502494650896497920,2461119.6472,13.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 502494650896497920 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:26.76 +73:55:10.8 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.19 05:22:24.96 +66:19:03.7
145.73041 16.39120 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 | 05:22:24.96 +66:19:03.7 (user input) | T | P | (position from user input) J-Ks=0.607+/-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,2461119.6472,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 13.19CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:22:24.96 +66:19:03.7 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
LU Cam,2461119.6472,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
LU Cam 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:58:17.58 +67:53:45.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.12 04:34:47.55 +66:05:05.8
143.01676 12.37132 galactic Cam Second-epoch detections are separated by 2.6" 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 | 04:34:47.55 +66:05:05.8 (user input) | T | P | (position from user input) J-Ks=0.421+/-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,2461119.6472,13.12,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:34:47.55 +66:05:05.8 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:27.18 +73:34:55.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1472* 03 12 38.28 +72 39 11.6 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
target,2461119.6472,12.95,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.95CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:12:38.28 +72:39:11.6 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1472* 03 18 08.68 +71 39 25.8 12.9 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:18:08.68 +71:39:25.8 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.03 05:44:28.49 +64:32:52.2
148.50341 17.55120 galactic Cam Second-epoch detections are separated by 1.7" 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 | Gaia DR3 287796069060255744 | 05:44:28.47 +64:32:27.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.390+/-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 287796069060255744,2461119.6472,13.03,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 287796069060255744 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:44:28.49 +64:32:52.2 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.93 04:11:33.37 +65:34:23.2
141.72238 10.29658 galactic Cam Second-epoch detections are separated by 0.9" 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 | 04:11:33.37 +65:34:23.2 (user input) | T | P | (position from user input) J-Ks=0.554+/-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,2461119.6472,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:11:33.37 +65:34:23.2 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1472* 03 17 10.56 +69 54 48.5 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 541454569818724864,2461119.6472,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 541454569818724864 20260320.1472 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:17:10.56 +69:54:48.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1472* 03 10 42.63 +73 30 53.5 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.81CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:10:42.63 +73:30:53.5 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:32:28.46 +67:14:27.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1472* 03 22 24.94 +73 47 02.3 12.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,12.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.82CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:22:24.94 +73:47:02.3 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:01.35 +69:29:05.8 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.92 04:54:50.39 +66:57:16.6
143.60802 14.47125 galactic Cam Second-epoch detections are separated by 0.3" 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 | 04:54:50.39 +66:57:16.6 (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,2461119.6472,12.92,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.92CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:54:50.39 +66:57:16.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.79 05:02:53.69 +65:01:14.4
145.71932 13.99947 galactic Cam Second-epoch detections are separated by 1.3" 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 | 05:02:53.69 +65:01:14.4 (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,2461119.6472,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:02:53.69 +65:01:14.4 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.96 04:32:07.11 +69:05:37.1
140.51502 14.15691 galactic Cam Second-epoch detections are separated by 1.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:32:07.11 +69:05:37.1 (user input) | T | P | (position from user input) 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
target,2461119.6472,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:32:07.11 +69:05:37.1 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.79 04:02:19.67 +70:42:08.3
137.49274 13.44447 galactic Cam Second-epoch detections are separated by 0.7" 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 | 04:02:19.67 +70:42:08.3 (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,2461119.6472,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:02:19.67 +70:42:08.3 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.65 05:12:59.98 +68:41:28.7
143.12799 16.86576 galactic Cam Second-epoch detections are separated by 0.4" 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 | 05:12:59.98 +68:41:28.7 (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,2461119.6472,12.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:12:59.98 +68:41:28.7 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1472* 03 13 13.23 +72 32 45.4 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,2461119.6472,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:13:13.23 +72:32:45.4 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1472* 03 15 24.46 +73 35 27.6 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,12.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:15:24.46 +73:35:27.6 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1472* 03 08 09.62 +72 20 39.1 12.3 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,2461119.6472,12.34,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.34CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:09.62 +72:20:39.1 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.38 04:22:14.21 +65:32:26.1
142.54040 11.05518 galactic Cam Second-epoch detections are separated by 0.6" 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 | 04:22:14.21 +65:32:26.1 (user input) | T | P | (position from user input) J-Ks=0.634+/-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
target,2461119.6472,12.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.38CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:22:14.21 +65:32:26.1 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1472* 03 07 49.50 +72 26 25.5 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
target,2461119.6472,12.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.39CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:07:49.50 +72:26:25.5 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1472* 03 12 19.68 +71 19 44.4 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:12:19.68 +71:19:44.4 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1472* 03 08 28.72 +72 22 00.5 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,12.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:28.72 +72:22:00.5 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1472* 03 13 32.43 +71 53 25.2 12.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,12.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:13:32.43 +71:53:25.2 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1472* 03 15 15.25 +70 34 15.1 12.2 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,2461119.6472,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.17CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:15:15.25 +70:34:15.1 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 489750486496727680,2461119.6472,12.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 489750486496727680 20260320.1472 12.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:20:32.42 +67:29:55.0 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:36:17.78 +72:45:20.9 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.17 03:14:45.18 +72:01:17.1
133.58378 12.18075 galactic Cas Second-epoch detections are separated by 2.7" and 6.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 543941600697991424 | 03:14:43.56 +72:01:14.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1472* 03 14 45.18 +72 01 17.1 12.2 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
Gaia DR3 543941600697991424,2461119.6472,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543941600697991424 20260320.1472 12.17CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:14:45.18 +72:01:17.1 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.06 03:08:57.58 +72:54:01.9
132.73135 12.70066 galactic Cas Second-epoch detections are separated by 1.2" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 544225442198980096 | 03:08:59.16 +72:54:03.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1472* 03 08 57.58 +72 54 01.9 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544225442198980096,2461119.6472,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544225442198980096 20260320.1472 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:08:57.58 +72:54:01.9 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.06 03:14:47.53 +73:15:58.9
132.90465 13.23480 galactic Cas Second-epoch detections are separated by 1.7" 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 544342127870595968 | 03:14:45.28 +73:15:56.8 (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!
TCP 2026 03 20.1472* 03 14 47.53 +73 15 58.9 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544342127870595968,2461119.6472,12.06,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544342127870595968 20260320.1472 12.06CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:14:47.53 +73:15:58.9 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 11.42 04:05:44.41 +69:16:50.2
138.70516 12.60126 galactic Cam Second-epoch detections are separated by 1.8" 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 | Gaia DR3 493935979369184384 | 04:05:40.89 +69:16:44.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.887+/-0.025 (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 493935979369184384,2461119.6472,11.42,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493935979369184384 20260320.1472 11.42CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:05:44.41 +69:16:50.2 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 11.28 03:45:58.45 +68:00:22.8
138.16786 10.46104 galactic Cam Second-epoch detections are separated by 1.4" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 493476112928592512 | 03:45:59.00 +68:00:23.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 493476112928592512,2461119.6472,11.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493476112928592512 20260320.1472 11.28CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:58.45 +68:00:22.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 11.13 03:10:42.06 +73:20:48.1
132.60488 13.14769 galactic Cas Second-epoch detections are separated by 0.7" 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 | Gaia DR3 544334950982181632 | 03:10:43.70 +73:20:52.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1472* 03 10 42.06 +73 20 48.1 11.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544334950982181632,2461119.6472,11.13,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544334950982181632 20260320.1472 11.13CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:10:42.06 +73:20:48.1 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 8.43 04:30:48.67 +64:51:50.5
143.66947 11.25192 galactic Cam Second-epoch detections are separated by 0.2" 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 | Gaia DR3 477013468924148736 | 04:30:48.65 +64:51:50.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: G0 1956PMcCO..13a....B AG+64 268 J-Ks=0.557+/-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
Gaia DR3 477013468924148736,2461119.6472,8.43,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 477013468924148736 20260320.1472 8.43CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:30:48.67 +64:51:50.5 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 10.90 03:53:34.78 +64:50:56.9
140.79156 8.49959 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 | Gaia DR3 489011374165131648 | 03:53:34.85 +64:50:56.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.318+/-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
Gaia DR3 489011374165131648,2461119.6472,10.90,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 489011374165131648 20260320.1472 10.90CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:34.78 +64:50:56.9 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 10.98 05:33:26.98 +65:17:16.9
147.24902 16.86066 galactic Cam Second-epoch detections are separated by 0.7" 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 | Gaia DR3 479901954687026560 | 05:33:25.74 +65:16:43.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.325+/-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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 479901954687026560,2461119.6472,10.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 479901954687026560 20260320.1472 10.98CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:33:26.98 +65:17:16.9 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 11.05 03:43:49.03 +64:45:07.2
140.03638 7.77141 galactic Cam Second-epoch detections are separated by 0.2" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 488294316487226112 | 03:43:43.93 +64:44:50.5 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.245+/-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
Gaia DR3 488294316487226112,2461119.6472,11.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 488294316487226112 20260320.1472 11.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:49.03 +64:45:07.2 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 11.23 04:00:27.78 +68:34:39.7
138.83340 11.76264 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 | Gaia DR3 493787098621550976 | 04:00:22.15 +68:34:24.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.187+/-0.050 (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 493787098621550976,2461119.6472,11.23,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493787098621550976 20260320.1472 11.23CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:00:27.78 +68:34:39.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 11.26 04:29:51.32 +65:59:10.2
142.75181 11.93087 galactic Cam Second-epoch detections are separated by 0.8" 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 477356104234708480 | 04:29:53.21 +65:59:34.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.353+/-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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 477356104234708480,2461119.6472,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 477356104234708480 20260320.1472 11.26CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:29:51.32 +65:59:10.2 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 11.57 04:42:14.52 +69:04:10.6
141.13399 14.83356 galactic Cam 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 | 04:42:14.52 +69:04:10.6 (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,2461119.6472,11.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 11.57CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:42:14.52 +69:04:10.6 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 11.68 04:18:40.67 +74:39:11.6
135.50228 17.10319 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 | 04:18:40.67 +74:39:11.6 (user input) | T | P | (position from user input) J-Ks=0.544+/-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,2461119.6472,11.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 11.68CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:18:40.67 +74:39:11.6 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 11.70 04:59:39.30 +71:29:48.0
140.02318 17.46046 galactic Cam Second-epoch detections are separated by 0.6" 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 | Gaia DR3 497551280978047488 | 04:59:30.37 +71:29:54.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: F2 1956PMcCO..13a....B AG+71 170 J-Ks=0.421+/-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
Gaia DR3 497551280978047488,2461119.6472,11.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 497551280978047488 20260320.1472 11.70CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:59:39.30 +71:29:48.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 11.82 05:46:27.89 +68:07:41.2
145.20034 19.29438 galactic Cam Second-epoch detections are separated by 1.2" 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 | Gaia DR3 481671859173539200 | 05:46:29.06 +68:08:10.9 (Gaia DR3) | DSCT/GDOR (local) | A (local) | Gaia3var=VARIABLE J-Ks=0.373+/-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
Gaia DR3 481671859173539200,2461119.6472,11.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 481671859173539200 20260320.1472 11.82CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:27.89 +68:07:41.2 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0418017+711356,2461119.6472,11.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0418017+711356 20260320.1472 11.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:18:00.86 +71:13:59.0 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 11.98 04:57:37.99 +70:38:35.3
140.65841 16.83840 galactic Cam Second-epoch detections are separated by 0.4" 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 | 04:57:37.99 +70:38:35.3 (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,2461119.6472,11.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 11.98CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:57:37.99 +70:38:35.3 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.45 05:17:15.95 +73:34:57.9
138.90548 19.68929 galactic Cam Second-epoch detections are separated by 2.0" 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 | 05:17:15.95 +73:34:57.9 (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,2461119.6472,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:15.95 +73:34:57.9 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.46 04:00:50.26 +67:35:24.1
139.53230 11.05035 galactic Cam Second-epoch detections are separated by 1.4" and 6.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 490306839381085952 | 04:00:57.56 +67:35:25.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.389+/-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
Gaia DR3 490306839381085952,2461119.6472,12.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 490306839381085952 20260320.1472 12.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:00:50.26 +67:35:24.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.59 04:27:04.11 +67:43:40.4
141.24403 12.90052 galactic Cam Second-epoch detections are separated by 0.7" 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 495750452730515584 | 04:27:00.65 +67:43:23.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.898+/-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 495750452730515584,2461119.6472,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 495750452730515584 20260320.1472 12.59CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:27:04.11 +67:43:40.4 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:29:19.00 +69:15:33.7 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,12.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:55:20.52 +64:07:13.5 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.66 04:50:16.69 +72:56:19.2
138.35515 17.71093 galactic Cam Second-epoch detections are separated by 0.7" 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 | 04:50:16.69 +72:56:19.2 (user input) | T | P | (position from user input) J-Ks=0.350+/-0.030 (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,2461119.6472,12.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:16.69 +72:56:19.2 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.58 04:50:31.26 +70:07:14.5
140.73309 16.04839 galactic Cam Second-epoch detections are separated by 0.6" 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 | 04:50:31.26 +70:07:14.5 (user input) | T | P | (position from user input) J-Ks=0.826+/-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!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,12.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:31.26 +70:07:14.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.69 03:57:23.35 +71:25:00.4
136.69399 13.70557 galactic Cam Second-epoch detections are separated by 2.0" and 6.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 495284156721043456 | 03:57:27.88 +71:25:33.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 495284156721043456,2461119.6472,12.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 495284156721043456 20260320.1472 12.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:57:23.35 +71:25:00.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,12.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:22.42 +72:53:50.5 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.81 05:53:03.71 +64:13:58.4
149.22543 18.24980 galactic Cam Second-epoch detections are separated by 1.8" 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 | 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 287049225785639808,2461119.6472,12.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 287049225785639808 20260320.1472 12.81CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:53:03.71 +64:13:58.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.78 05:21:43.12 +66:47:48.5
145.26439 16.57739 galactic Cam Second-epoch detections are separated by 1.1" 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 | 05:21:43.12 +66:47:48.5 (user input) | T | P | (position from user input) J-Ks=0.485+/-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,2461119.6472,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:21:43.12 +66:47:48.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:16:56.09 +69:09:47.9 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.86 04:55:33.01 +66:54:52.5
143.68402 14.50332 galactic Cam Second-epoch detections are separated by 0.9" 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 | 04:55:33.01 +66:54:52.5 (user input) | T | P | (position from user input) J-Ks=0.664+/-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,2461119.6472,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:55:33.01 +66:54:52.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.01 04:29:19.56 +69:31:53.2
140.00797 14.26123 galactic Cam Second-epoch detections are separated by 1.7" 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 | Large-amplitude variable Gaia DR2 496854912160414848 | 04:29:19.56 +69:31:53.2 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
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 496854912160414848,2461119.6472,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 496854912160414848 20260320.1472 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:29:19.56 +69:31:53.2 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:30.86 +72:51:34.2 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.00 04:20:01.12 +68:13:26.2
140.40926 12.75800 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 | 04:20:01.12 +68:13:26.2 (user input) | T | P | (position from user input) J-Ks=0.593+/-0.092 (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,2461119.6472,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:20:01.12 +68:13:26.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.96 04:45:55.16 +68:04:57.6
142.14776 14.48022 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 | Gaia DR3 495600369393497600 | 04:45:51.14 +68:05:31.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.436+/-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 495600369393497600,2461119.6472,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 495600369393497600 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:45:55.16 +68:04:57.6 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 498145085975528064,2461119.6472,13.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 498145085975528064 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:17:22.73 +71:24:55.0 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.98 04:14:47.99 +68:29:38.1
139.86635 12.60358 galactic Cam Second-epoch detections are separated by 1.9" 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 | Large-amplitude variable Gaia DR2 490781038127204608 | 04:14:42.98 +68:29:07.2 (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=1.073+/-0.031 (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
Large-amplitude variable Gaia DR2 490781038127204608,2461119.6472,12.98,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 490781038127204608 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:14:47.99 +68:29:38.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 12.96 05:29:55.17 +74:30:44.9
138.47340 20.89563 galactic Cam Second-epoch detections are separated by 4.4" 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 502792034430665088 | 05:29:44.31 +74:30:47.0 (Gaia DR3) | DSCT/GDOR (local) | A (local) | Gaia3var=VARIABLE SpType: A2 1956PMcCO..13a....B AG+74 124
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 502792034430665088,2461119.6472,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 502792034430665088 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:29:55.17 +74:30:44.9 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.04 05:03:33.84 +65:44:44.7
145.14899 14.47381 galactic Cam Second-epoch detections are separated by 3.5" 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 | 05:03:33.84 +65:44:44.7 (user input) | T | P | (position from user input) J-Ks=0.481+/-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,2461119.6472,13.04,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:33.84 +65:44:44.7 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.28 05:24:01.23 +71:37:20.2
140.97849 19.16421 galactic Cam Second-epoch detections are separated by 1.9" 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 | 05:24:01.23 +71:37:20.2 (user input) | T | P | (position from user input) J-Ks=0.324+/-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,2461119.6472,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:24:01.23 +71:37:20.2 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,13.14,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 13.14CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:05:07.94 +67:40:12.8 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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+703407.7,2461119.6472,13.18,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J051555.95+703407.7 20260320.1472 13.18CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:56.81 +70:34:25.3 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.08 04:38:34.60 +65:24:55.1
143.79562 12.22899 galactic Cam Second-epoch detections are separated by 3.9" 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 | 04:38:34.60 +65:24:55.1 (user input) | T | P | (position from user input) J-Ks=0.756+/-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
target,2461119.6472,13.08,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 13.08CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:38:34.60 +65:24:55.1 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.28 05:07:59.82 +65:47:22.8
145.37803 14.87347 galactic Cam Second-epoch detections are separated by 3.6" 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 | Gaia DR3 479590827261511936 | 05:08:04.72 +65:47:30.9 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.406+/-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 479590827261511936,2461119.6472,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 479590827261511936 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:07:59.82 +65:47:22.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.15 05:39:11.34 +68:47:03.4
144.26723 18.97901 galactic Cam Second-epoch detections are separated by 2.0" 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 | 05:39:11.34 +68:47:03.4 (user input) | T | P | (position from user input) J-Ks=0.351+/-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,2461119.6472,13.15,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:39:11.34 +68:47:03.4 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.27 04:59:15.34 +65:54:52.3
144.74315 14.21234 galactic Cam Second-epoch detections are separated by 0.3" 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 482548032501399296 | 04:59:17.04 +65:54:13.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.389+/-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 482548032501399296,2461119.6472,13.27,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 482548032501399296 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:59:15.34 +65:54:52.3 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.28 05:01:54.54 +71:44:42.3
139.91245 17.74705 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 | Gaia DR3 497558393443830656 | 05:01:57.82 +71:45:16.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.454+/-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
Gaia DR3 497558393443830656,2461119.6472,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 497558393443830656 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:01:54.54 +71:44:42.3 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:36:09.32 +69:59:53.6 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.24 04:58:10.25 +65:24:26.3
145.09807 13.82352 galactic Cam Second-epoch detections are separated by 2.6" 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 | 04:58:10.25 +65:24:26.3 (user input) | T | P | (position from user input) J-Ks=0.395+/-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,2461119.6472,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:58:10.25 +65:24:26.3 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:34.32 +67:41:09.7 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.30 05:06:10.92 +64:52:32.5
146.04739 14.20162 galactic Cam Second-epoch detections are separated by 2.2" and 6.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:06:10.92 +64:52:32.5 (user input) | T | P | (position from user input) J-Ks=0.492+/-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,2461119.6472,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:06:10.92 +64:52:32.5 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.24 05:01:07.01 +70:03:24.2
141.33588 16.74368 galactic Cam Second-epoch detections are separated by 1.1" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:01:07.01 +70:03:24.2 (user input) | T | P | (position from user input) J-Ks=0.426+/-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
target,2461119.6472,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 13.24CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:01:07.01 +70:03:24.2 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.50 06:01:10.95 +71:55:17.3
141.98868 21.92520 galactic Cam Second-epoch detections are separated by 1.7" 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 | 06:01:10.95 +71:55:17.3 (user input) | T | P | (position from user input) J-Ks=0.644+/-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,2461119.6472,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:10.95 +71:55:17.3 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:32:40.04 +65:00:00.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,13.30,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:41:41.12 +70:56:51.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:11:19.27 +72:08:07.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 489917887142564224,2461119.6472,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 489917887142564224 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:02:25.59 +66:01:46.0 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.56 04:51:35.87 +65:30:23.6
144.59484 13.33726 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 | ATO J072.9041+65.4984 | 04:51:35.87 +65:30:23.6 (user input) | dubious (ATLAS) | (ATLAS) | (position from user input) J-Ks=0.569+/-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
ATO J072.9041+65.4984,2461119.6472,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J072.9041+65.4984 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:51:35.87 +65:30:23.6 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.36 04:43:20.69 +72:22:21.8
138.50184 16.95753 galactic Cam Second-epoch detections are separated by 1.2" 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 | Gaia DR3 500791335585802496 | 04:43:18.83 +72:21:41.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.606+/-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 500791335585802496,2461119.6472,13.36,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 500791335585802496 20260320.1472 13.36CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:43:20.69 +72:22:21.8 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.48 04:32:18.16 +66:04:29.9
142.85383 12.17523 galactic Cam Second-epoch detections are separated by 2.6" 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 | 04:32:18.16 +66:04:29.9 (user input) | T | P | (position from user input) J-Ks=0.533+/-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,2461119.6472,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:32:18.16 +66:04:29.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.52 05:20:32.39 +65:19:26.7
146.51166 15.71261 galactic Cam Second-epoch detections are separated by 1.8" 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 | 05:20:32.39 +65:19:26.7 (user input) | T | P | (position from user input) J-Ks=0.597+/-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,2461119.6472,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:20:32.39 +65:19:26.7 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:41:55.49 +65:26:14.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.49 05:48:13.93 +67:04:45.2
146.28135 19.00175 galactic Cam Second-epoch detections are separated by 1.5" 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 | 05:48:13.93 +67:04:45.2 (user input) | T | P | (position from user input) J-Ks=0.470+/-0.052 (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,2461119.6472,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:13.93 +67:04:45.2 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J040209.43+704538.1,2461119.6472,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ZTF J040209.43+704538.1 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:02:09.32 +70:45:37.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.49 04:41:09.33 +67:50:57.0
142.04628 13.98579 galactic Cam Second-epoch detections are separated by 0.5" 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 | Gaia DR3 495571163616051456 | 04:41:05.49 +67:51:29.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.409+/-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 495571163616051456,2461119.6472,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 495571163616051456 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:41:09.33 +67:50:57.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.56 04:12:01.89 +69:32:11.6
138.93247 13.16904 galactic Cam Second-epoch detections are separated by 0.7" 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 | 04:12:01.89 +69:32:11.6 (user input) | T | P | (position from user input) J-Ks=0.343+/-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,2461119.6472,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:12:01.89 +69:32:11.6 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.62 04:06:53.12 +65:28:30.0
141.43367 9.89299 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 | 04:06:53.12 +65:28:30.0 (user input) | T | P | (position from user input) J-Ks=0.552+/-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,2461119.6472,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:06:53.12 +65:28:30.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.54 05:20:36.05 +66:22:28.4
145.58184 16.26449 galactic Cam Second-epoch detections are separated by 1.3" 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 | 05:20:36.05 +66:22:28.4 (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,2461119.6472,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:20:36.05 +66:22:28.4 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:39:49.20 +67:53:55.8 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.32 05:54:24.56 +67:33:40.0
146.07605 19.74284 galactic Cam Second-epoch detections are separated by 2.8" 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 | 05:54:24.56 +67:33:40.0 (user input) | T | P | (position from user input) J-Ks=0.350+/-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,2461119.6472,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:54:24.56 +67:33:40.0 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.70 04:56:17.91 +70:32:23.5
140.67947 16.68822 galactic Cam Second-epoch detections are separated by 1.3" 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 | 04:56:17.91 +70:32:23.5 (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,2461119.6472,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:17.91 +70:32:23.5 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.38 04:40:44.63 +71:13:49.0
139.30502 16.08950 galactic Cam 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 | Gaia DR3 500472374135333248 | 04:40:44.02 +71:13:03.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.433+/-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 500472374135333248,2461119.6472,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 500472374135333248 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:40:44.63 +71:13:49.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.64 05:19:50.18 +70:16:36.3
142.03401 18.20135 galactic Cam Second-epoch detections are separated by 4.4" 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 | 05:19:50.18 +70:16:36.3 (user input) | T | P | (position from user input) J-Ks=0.594+/-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,2461119.6472,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:19:50.18 +70:16:36.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 480527920400518784,2461119.6472,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 480527920400518784 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:46:48.60 +66:28:28.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.57 06:02:49.55 +66:59:08.9
146.97531 20.26971 galactic Cam Second-epoch detections are separated by 1.0" 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 | Gaia DR3 1104912364469817088 | 06:02:56.73 +66:58:53.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.449+/-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
Gaia DR3 1104912364469817088,2461119.6472,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1104912364469817088 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:02:49.55 +66:59:08.9 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 483095005176245376,2461119.6472,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 483095005176245376 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:35:53.88 +65:39:42.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.71 06:09:07.02 +72:22:40.1
141.74394 22.65086 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 | 06:09:07.02 +72:22:40.1 (user input) | T | P | (position from user input) J-Ks=0.746+/-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,2461119.6472,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:09:07.02 +72:22:40.1 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.72 05:06:50.26 +64:51:24.5
146.10418 14.24824 galactic Cam Second-epoch detections are separated by 1.8" 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 | 05:06:50.26 +64:51:24.5 (user input) | T | P | (position from user input) J-Ks=0.370+/-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,2461119.6472,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:06:50.26 +64:51:24.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.73 04:05:46.24 +69:03:16.9
138.86540 12.43823 galactic Cam Second-epoch detections are separated by 3.0" 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 | Gaia DR3 493824692474024832 | 04:05:52.19 +69:03:50.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 493824692474024832,2461119.6472,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493824692474024832 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:05:46.24 +69:03:16.9 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.62 05:25:27.13 +68:03:13.8
144.31833 17.52096 galactic Cam Second-epoch detections are separated by 0.4" 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 | 05:25:27.13 +68:03:13.8 (user input) | T | P | (position from user input) J-Ks=0.384+/-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,2461119.6472,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:25:27.13 +68:03:13.8 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 482088471000996736,2461119.6472,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 482088471000996736 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:54:44.70 +65:04:14.9 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.65 05:00:53.03 +64:54:36.1
145.68480 13.76203 galactic Cam Second-epoch detections are separated by 0.8" and 6.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:00:53.03 +64:54:36.1 (user input) | T | P | (position from user input) J-Ks=0.374+/-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,2461119.6472,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:00:53.03 +64:54:36.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J045246.90+674923.1,2461119.6472,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ASASSN-V J045246.90+674923.1 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:52:46.89 +67:49:23.1 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 486057192579327872,2461119.6472,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 486057192579327872 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:48:20.98 +70:52:48.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:15:09.85 +69:56:55.4 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.68 04:13:11.73 +67:46:21.7
140.27768 11.98637 galactic Cam Second-epoch detections are separated by 1.0" 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 | 04:13:11.73 +67:46:21.7 (user input) | T | P | (position from user input) J-Ks=0.592+/-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,2461119.6472,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:13:11.73 +67:46:21.7 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.63 04:25:21.76 +65:57:39.6
142.45443 11.57734 galactic Cam Second-epoch detections are separated by 1.0" 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 | 04:25:21.76 +65:57:39.6 (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,2461119.6472,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:21.76 +65:57:39.6 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:07:07.42 +71:41:37.3 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.54 03:58:05.38 +65:01:43.4
141.04137 8.94609 galactic Cam Second-epoch detections are separated by 2.5" 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 | 03:58:05.38 +65:01:43.4 (user input) | T | P | (position from user input) J-Ks=0.930+/-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
target,2461119.6472,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:58:05.38 +65:01:43.4 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.69 05:11:49.87 +65:47:00.4
145.60887 15.19734 galactic Cam Second-epoch detections are separated by 1.0" 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 | 05:11:49.87 +65:47:00.4 (user input) | T | P | (position from user input) J-Ks=0.516+/-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,2461119.6472,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:11:49.87 +65:47:00.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.66 05:06:00.80 +66:58:52.0
144.24087 15.37735 galactic Cam 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 | 05:06:00.80 +66:58:52.0 (user input) | T | P | (position from user input) J-Ks=0.652+/-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,2461119.6472,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:06:00.80 +66:58:52.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.69 05:19:54.25 +71:34:18.4
140.85586 18.85656 galactic Cam Second-epoch detections are separated by 3.1" 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 | 05:19:54.25 +71:34:18.4 (user input) | T | P | (position from user input) J-Ks=0.835+/-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,2461119.6472,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:19:54.25 +71:34:18.4 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.62 04:29:42.40 +65:27:15.7
143.14374 11.56235 galactic Cam Second-epoch detections are separated by 1.4" 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 | 04:29:42.40 +65:27:15.7 (user input) | T | P | (position from user input) J-Ks=0.488+/-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,2461119.6472,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:29:42.40 +65:27:15.7 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461119.6472,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:27:50.85 +66:14:55.8 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 550012725949488768,2461119.6472,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 550012725949488768 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:57.70 +74:11:24.3 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.72 04:42:25.97 +67:11:09.6
142.65438 13.66017 galactic Cam Second-epoch detections are separated by 0.8" 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 | 04:42:25.97 +67:11:09.6 (user input) | T | P | (position from user input) J-Ks=0.723+/-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,2461119.6472,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:42:25.97 +67:11:09.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.78 04:42:27.84 +68:36:52.3
141.51303 14.56322 galactic Cam Second-epoch detections are separated by 0.9" 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 | 04:42:27.84 +68:36:52.3 (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,2461119.6472,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:42:27.84 +68:36:52.3 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.69 04:51:07.98 +69:25:24.9
141.34586 15.67246 galactic Cam Second-epoch detections are separated by 0.9" 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 496296841290259328 | 04:51:10.13 +69:26:06.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.579+/-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
Gaia DR3 496296841290259328,2461119.6472,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 496296841290259328 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:51:07.98 +69:25:24.9 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.76 03:57:36.41 +67:28:34.5
139.37351 10.76068 galactic Cam Second-epoch detections are separated by 2.0" 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 | 03:57:36.41 +67:28:34.5 (user input) | T | P | (position from user input) J-Ks=0.549+/-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,2461119.6472,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:57:36.41 +67:28:34.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 485749982159123456,2461119.6472,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 485749982159123456 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:31:40.78 +70:19:44.6 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 13.73 05:45:20.27 +72:47:19.3
140.63862 21.14078 galactic Cam Second-epoch detections are separated by 1.0" 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 | 05:45:20.27 +72:47:19.3 (user input) | T | P | (position from user input) J-Ks=0.563+/-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,2461119.6472,13.73,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260320.1472 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:45:20.27 +72:47:19.3 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
NSVS J0405390+661955,2461119.6472,11.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0405390+661955 20260320.1472 11.49CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:05:39.55 +66:19:58.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 20.1472 2461119.6472 10.51 06:23:58.24 +72:38:04.4
141.82781 23.79347 galactic Cam Second-epoch detections are separated by 0.2" 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 | Gaia DR3 1113724400409693952 | 06:23:57.92 +72:38:03.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.277+/-0.033 (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 1113724400409693952,2461119.6472,10.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 1113724400409693952 20260320.1472 10.51CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:23:58.24 +72:38:04.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 20.1472* 03 28 21.89 +70 57 01.0 11.5 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
NSVS J0328205+705703,2461119.6472,11.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
NSVS J0328205+705703 20260320.1472 11.50CV 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:28:21.89 +70:57:01.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20_00sec_-14_90C_LIGHT_0101_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20_00sec_-14_90C_LIGHT_0100_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Last image: 2461119.64743428 20.03.2026 03:32:08.322 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 23
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.62
Magnitude-Size filter: Disabled
For each source choose aperture with the smallest scatter: YES
Photometric errors rescaling: NO
Number of identified bad images: 0
Number of SysRem iterations: 0
User-specified moving object: none
Computation time: 4 seconds
Number of parallel threads: 24
SExtractor parameter file: default.sex
Some important SExtractor parameters:
DETECT_MINAREA 10.0 # minimum number of pixels above threshold
DETECT_THRESH 10.0 # or , in mag.arcsec-2
ANALYSIS_THRESH 10.0 # or , in mag.arcsec-2
SATUR_LEVEL 55000.0 # level (in ADUs) at which arises saturation
GAIN 0.37 # detector gain in e-/ADU
Total objects detected (at least 2 times): 17399
Objects passed selection criteria: 17384
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 16068.5
Average stars matched: 15390.5 (95.7806 %)
Memory usage VmPeak: 121060 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 22:56:54 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Last image: 2461119.64743428 20.03.2026 03:32:08.322 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 273
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: 41 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): 111990
Objects passed selection criteria: 111735
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 102619
Average stars matched: 98256.5 (95.7486 %)
Memory usage VmPeak: 2001608 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Mar 11 15:05:24 CDT 2026
VaST build number 1.0rc88-349-g45f03b26
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Thu Mar 19 22:58:29 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
SExtractor catalog cache: saved Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat to cache
SExtractor catalog cache: saved Cam-06-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.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: 2461119.64687559
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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits exists and is non-empty
Saving wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits to local_wcs_cache/
'wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> 'local_wcs_cache/wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits'
wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits exists and is non-empty
Saving wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits to local_wcs_cache/
'wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> 'local_wcs_cache/wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits'
wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits'
wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits'
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:47:48.196 +70:00:29.12
Second-epoch image center 04:47:58.513 +69:59:56.01
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:47:48.196 +70:00:29.12
Second-epoch image center 04:47:57.058 +70:00:31.53
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:47:58.513 +69:59:56.01
Second-epoch second image center 04:47:57.058 +70:00:31.53
Angular distance between the image centers 0.01008 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits &> /tmp/tmp.bZbyW7Pp9V
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_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-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits &> /tmp/tmp.2vUpJWq0hk
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits &> /tmp/tmp.HoHMAgMa93
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits &> /tmp/tmp.UVRx0sgUNg
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-06-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Found non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
The reference image (wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits) and catalog (wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat) found
'wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 58 out of 16183 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.881698
a=0.000000 b=1.000000 c=22.881698
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.26
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.26
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 22 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
2.1 pix Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
2.5 pix fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
2.5 pix fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
Limiting magnitude estimates:
15.3 mag. Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
15.2 mag. Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
15.1 mag. fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
15.1 mag. fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
All-image limiting magnitude estimate: 15.1 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.bZbyW7Pp9V (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> 'wcs_Cam-06-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits -region wcs_Cam-06-Q2b1x1_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-Q2b1x1_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.2vUpJWq0hk (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> 'wcs_Cam-06-Q2b1x1_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-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits -region wcs_Cam-06-Q2b1x1_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-Q2b1x1_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.HoHMAgMa93 (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1016, passed=16143
Got 16143 stars (including 15115 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits.cat
util/solve_plate_with_UCAC5 got 16143 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 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: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.57"
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: 0.57"
Estimated accuracy of the plate solution: 0.60"
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-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits -region wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.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.UVRx0sgUNg (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1022, passed=16136
Got 16136 stars (including 15106 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits.cat
util/solve_plate_with_UCAC5 got 16136 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 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: 0.58"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.58"
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: 0.58"
Estimated accuracy of the plate solution: 0.60"
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-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits -region wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits'
Saving fully-calibrated image wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits'
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits'
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits'
Preparing the HTML report for the field Cam-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out21029.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21032.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21413.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21488.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21527.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21531.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21566.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21574.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21585.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21611.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21618.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21622.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21628.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21630.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21631.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21638.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21652.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21670.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21675.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21680.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21699.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 3s
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: 1s
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Considering the candidate 21029_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21029_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 05:20:10.31 +71:33:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.08, MAG_FAINT_SEARCH_LIMIT=13.06)GAIADR2_OUTPUT=# 0.707 498147899176343936 080.04274431906 +71.56495450163 11.8098 11.0125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.707#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21032_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21032_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:23:15.89 +65:09:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.85, MAG_FAINT_SEARCH_LIMIT=12.83)GAIADR2_OUTPUT=# 0.838 477165579483957504 065.81619667352 +65.15618392704 11.3828 10.4592 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.838#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21413_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21413_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:33:19.92 +70:27:45.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.74, MAG_FAINT_SEARCH_LIMIT=12.72)GAIADR2_OUTPUT=# 0.760 497068251776071296 068.33335138020 +70.46251921137 11.6749 10.9767 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.760#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21488_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21488_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:42:42.95 +64:44:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.98, MAG_FAINT_SEARCH_LIMIT=12.96)GAIADR2_OUTPUT=# 4.601 488212201011316480 055.67736897839 +64.73766679550 11.6343 10.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.601#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21527_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21527_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:44:01.19 +69:06:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.796 496311856496236800 071.00549774881 +69.10413684241 12.0561 11.5968 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.796#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21531_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21531_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:37:54.00 +71:27:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.685 500535802212355456 069.47518647410 +71.45454129490 11.9885 11.5352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.685#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21566_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21566_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:54:25.64 +69:35:33.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.07, MAG_FAINT_SEARCH_LIMIT=13.05)GAIADR2_OUTPUT=# 0.284 496304984544663168 073.60700128984 +69.59244696143 12.0245 11.5664 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.284#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21574_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21574_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:50:20.63 +68:09:05.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 0.204 495967984234117504 072.58584113756 +68.15164736946 12.0959 11.3506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21585_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21585_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:53:34.81 +64:50:57.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.421 489011374165131648 058.39519762886 +64.84912588101 12.0684 11.4023 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.421#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21611_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21611_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:37:48.89 +69:31:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.519 496770352844471040 069.45372612713 +69.52721705564 10.4768 9.0408 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.519#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21618_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21618_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 05:15:02.70 +73:00:52.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.20, MAG_FAINT_SEARCH_LIMIT=13.18)GAIADR2_OUTPUT=# 0.475 499272768290947328 078.76097407482 +73.01458988992 12.0140 11.2520 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.475#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21622_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21622_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:43:49.04 +64:45:07.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 1.448 488294350846964352 055.95512817238 +64.75186674570 12.2514 11.6869 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.448#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21628_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21628_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:58:29.00 +70:11:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.453 496466986416075008 074.62084971996 +70.19715214814 12.1331 11.6663 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.453#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21630_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21630_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:44:31.42 +72:48:36.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 0.430 500908669794258688 071.13116150341 +72.81009943899 10.8924 9.5397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.430#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21631_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21631_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:53:21.87 +69:39:47.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.23, MAG_FAINT_SEARCH_LIMIT=13.21)GAIADR2_OUTPUT=# 0.410 496309657472523264 073.34089644158 +69.66338715258 12.1163 11.5643 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.410#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21638_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21638_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 05:04:24.09 +69:47:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 0.129 496231587848912128 076.10027246800 +69.79728243252 12.0807 11.4351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.129#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21652_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21652_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:52:33.26 +69:03:26.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.31, MAG_FAINT_SEARCH_LIMIT=13.29)GAIADR2_OUTPUT=# 0.437 496085769416751744 073.13874825646 +69.05725488567 12.1207 11.4710 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.437#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21655_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21655_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:13:20.11 +72:06:36.1 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 21670_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21670_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 05:00:59.66 +73:20:54.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.243 502441736899623936 075.24850239058 +73.34851992498 12.2344 11.7708 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.243#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21675_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21675_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 05:08:42.21 +70:40:44.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.32, MAG_FAINT_SEARCH_LIMIT=13.30)GAIADR2_OUTPUT=# 0.790 497961123936904320 077.17528803194 +70.67887022278 12.3427 11.9350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.790#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21680_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21680_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 05:11:09.21 +70:03:59.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.339 497727817015043456 077.78817496843 +70.06654604345 12.3278 11.9209 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.339#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 21699_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 21699_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 05:13:40.37 +67:24:52.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.171 484436203203883904 078.41815276575 +67.41445742491 12.0905 11.3877 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.171#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: 4s
Prepared the HTML report for the field Cam-06-Q2b1x1 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 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
SExtractor catalog cache: saved Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat to cache
SExtractor catalog cache: saved Cam-06-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Creating symlink local_wcs_cache/wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits exists and is non-empty
wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits exists and is non-empty
wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits exists and is non-empty
wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits exists and is non-empty
The image scale is 5.84"/pix, setting the soft and hard astrometric limits for filtering second-epoch detections: 5.8" and 8.8"
###################################
# Check the image center offset between the reference and the first second-epoch image (pointing accuracy)
Reference image center 04:47:48.196 +70:00:29.12
Second-epoch image center 04:47:58.513 +69:59:56.01
Angular distance between the image centers 0.02 deg.
Soft limit: 0.50 deg. Hard limit: 1.00 deg.
###################################
###################################
# Check the image center offset between the reference and the second second-epoch image (pointing accuracy)
Reference image center 04:47:48.196 +70:00:29.12
Second-epoch image center 04:47:57.058 +70:00:31.53
Angular distance between the image centers 0.01 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:47:58.513 +69:59:56.01
Second-epoch second image center 04:47:57.058 +70:00:31.53
Angular distance between the image centers 0.01008 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits &> /tmp/tmp.0TLlfAbqAo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_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-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits &> /tmp/tmp.MgOUzlkRw4
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits &> /tmp/tmp.F5ZT3bGD5u
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits &> /tmp/tmp.CDojoujNnT
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-06-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Found non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
The reference image (wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits) and catalog (wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat) found
'wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 85 out of 113524 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.485424
a=0.000000 b=1.000000 c=21.485424
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.18
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.18
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 212 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
1.9 pix Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
2.4 pix fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
2.4 pix fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
Limiting magnitude estimates:
14.2 mag. Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
14.2 mag. Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
14.0 mag. fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
14.0 mag. fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
All-image limiting magnitude estimate: 14.0 (SNR ) 13.3 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.0TLlfAbqAo (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> 'wcs_Cam-06-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits -region wcs_Cam-06-Q2b1x1_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-Q2b1x1_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.MgOUzlkRw4 (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> 'wcs_Cam-06-Q2b1x1_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-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_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-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits -region wcs_Cam-06-Q2b1x1_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-Q2b1x1_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.F5ZT3bGD5u (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=24, blended=7959, passed=93123
Got 93123 stars (including 85060 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits.cat
util/solve_plate_with_UCAC5 got 93123 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 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 965 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: 0.55"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.53"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.53"
Estimated accuracy of the plate solution: 0.55"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits -region wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.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.CDojoujNnT (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=28, blended=8108, passed=93864
Got 93864 stars (including 85640 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits.cat
util/solve_plate_with_UCAC5 got 93864 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.3'
Seting catalog search parameters based on the expected field of view 937.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013018 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010414 (37.5 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 967 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: 0.56"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.54"
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 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.54"
Estimated accuracy of the plate solution: 0.56"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits -region wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Saving fully-calibrated image wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-31-20_20.00sec_-14.90C_LIGHT_0100.fits
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-19_CI_Cam-06-Q2b1x1_225345_TTUQ2b1x1_2515_jXp67YP6/wcs_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101.fits
Preparing the HTML report for the field Cam-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out132977.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133001.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133002.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133031.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133040.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133043.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133045.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133057.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133058.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133059.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133062.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133063.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133064.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133065.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133072.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133073.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133074.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133078.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133086.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133092.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133095.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133104.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133118.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133128.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133132.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133136.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133137.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133160.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133170.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133171.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133173.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133174.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133175.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133179.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133180.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133187.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133188.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133189.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133645.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135184.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135331.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out136075.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out136892.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out136895.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137012.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137048.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137437.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137572.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137607.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out137694.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_apass.txt__out133186.dat to exclusion_list_apass.txt
Adding exclusion_list_apass.txt__out133190.dat to exclusion_list_apass.txt
Adding exclusion_list_local.txt__out02641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132951.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132955.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132963.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132965.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132973.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132987.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132999.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133012.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133016.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133018.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133019.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133024.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133026.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133029.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__out133037.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133050.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__out133076.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133082.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133091.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133101.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133110.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133113.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133114.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133115.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133119.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133134.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133135.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133141.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133151.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133153.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133178.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133182.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133183.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133252.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133730.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133786.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133897.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134220.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134307.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134372.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134427.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134556.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134645.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135231.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135324.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135334.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135478.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135583.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135614.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135746.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135850.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135944.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136005.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136111.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136248.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136259.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136284.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136305.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136325.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136327.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136470.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136473.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136532.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136599.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136693.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136796.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136833.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136845.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136853.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136867.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136868.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136876.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136881.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136943.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136981.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137044.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137088.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137187.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137239.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137265.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137306.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137320.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137322.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137330.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137353.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137357.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137366.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137371.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137384.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137406.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137409.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137417.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137418.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137423.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137424.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137434.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137472.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137485.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137503.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137505.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137524.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137543.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137545.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137560.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137575.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137604.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137609.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137635.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137650.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137652.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137658.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137682.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137689.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out137720.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out43023.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out90043.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 198s
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: 104s
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Considering the candidate 132951_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 132951_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 132955_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 132955_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 132959_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 132959_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 132960_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 132960_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 132963_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 132963_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 132965_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 132965_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 132969_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 132969_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 132973_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 132973_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 132974_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 132974_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 132975_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 132975_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
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Considering the candidate 132977_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 132977_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:33:39.68 +67:26:19.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.28, MAG_FAINT_SEARCH_LIMIT=14.26)GAIADR2_OUTPUT=# 4.921 492001152439223296 053.41889458862 +67.43882008749 13.9629 13.2010 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.921#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132980_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 132980_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (10.0") between the two second-epoch detections
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Considering the candidate 132983_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 132983_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 132984_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 132984_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 132985_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 132985_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 132987_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 132987_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 132990_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 132990_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 132998_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 132998_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 132999_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 132999_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133001_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133001_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:23:43.88 +73:07:01.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.99, MAG_FAINT_SEARCH_LIMIT=13.97)GAIADR2_OUTPUT=# 3.376 544466342622460800 050.93478628433 +73.11769114832 13.5763 12.7164 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.376#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133002_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133002_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:21:53.43 +70:32:48.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.09, MAG_FAINT_SEARCH_LIMIT=14.07)GAIADR2_OUTPUT=# 2.734 542979218786639488 050.47476422262 +70.54706844758 13.7763 12.9997 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.734#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133012_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133012_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133016_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133016_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133018_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133018_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133019_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133019_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133021_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133021_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133024_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133024_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133026_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133026_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133029_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133029_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133031_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133031_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:16:51.85 +72:56:34.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 2.498 544261318063064064 049.21397425752 +72.94263492554 13.3465 12.6722 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.498#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133032_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133032_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133035_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133035_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133037_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133037_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133038_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133038_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133040_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133040_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:15:33.28 +73:41:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.76, MAG_FAINT_SEARCH_LIMIT=13.74)GAIADR2_OUTPUT=# 3.840 544369242001028480 048.88528058165 +73.69457198956 13.2665 12.4916 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.840#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133042_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133042_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (9.8") between the two second-epoch detections
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Considering the candidate 133043_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133043_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:23:20.77 +73:18:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.86, MAG_FAINT_SEARCH_LIMIT=13.84)GAIADR2_OUTPUT=# 2.484 544659233897595136 050.83463282863 +73.31675266415 13.4270 12.6876 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.484#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133045_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133045_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:38:31.55 +64:41:41.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 4.148 488398735731763584 054.63050281062 +64.69375601509 13.3846 12.6622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.148#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133048_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133048_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:15:11.37 +72:34:39.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.66, MAG_FAINT_SEARCH_LIMIT=13.64)GAIADR2_OUTPUT=# 2.886 544238468837207680 048.79882175047 +72.57842472243 13.3105 12.6352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.886#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133050_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133050_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133055_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133055_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133056_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133056_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133057_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133057_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:15:37.94 +71:13:02.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.68, MAG_FAINT_SEARCH_LIMIT=13.66)GAIADR2_OUTPUT=# 4.022 543820379541349632 048.90508012585 +71.21666255890 13.3959 12.7232 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.022#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133058_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133058_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:11:38.01 +65:34:43.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.79, MAG_FAINT_SEARCH_LIMIT=13.77)GAIADR2_OUTPUT=# 1.954 489292608623166208 062.90935278958 +65.57830450443 13.4570 12.1686 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.954#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133059_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133059_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:15:52.95 +72:53:43.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 2.621 544260076815353344 048.97279514828 +72.89587786500 13.1123 12.3794 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.621#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133062_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133062_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:19:11.94 +73:23:11.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.65, MAG_FAINT_SEARCH_LIMIT=13.63)GAIADR2_OUTPUT=# 1.072 544301209719204992 049.80011720867 +73.38630459938 13.4987 12.8676 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.072#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133063_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133063_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:33:26.05 +66:19:23.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.64, MAG_FAINT_SEARCH_LIMIT=13.62)GAIADR2_OUTPUT=# 2.356 491594230058078720 053.35703431321 +66.32283430031 13.4739 12.5750 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.356#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133064_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133064_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:19:05.63 +70:57:07.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.62, MAG_FAINT_SEARCH_LIMIT=13.60)GAIADR2_OUTPUT=# 2.393 543051198141608704 049.77501025085 +70.95237504462 13.3280 12.6841 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.393#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133065_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133065_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:27:03.01 +73:23:19.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 1.272 544477337738674432 051.76346298820 +73.38898556231 13.4158 12.7798 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.272#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133067_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133067_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (11.8") between the two second-epoch detections
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Considering the candidate 133072_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133072_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:14:37.12 +70:34:53.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.77, MAG_FAINT_SEARCH_LIMIT=13.75)GAIADR2_OUTPUT=# 4.713 541537724683093120 048.65118618315 +70.58225105085 13.4664 12.7064 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.713#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133073_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133073_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:19:41.85 +73:24:24.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.63, MAG_FAINT_SEARCH_LIMIT=13.61)GAIADR2_OUTPUT=# 4.793 544301312798414080 049.91971457948 +73.40689707520 13.2190 12.2790 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.793#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133074_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133074_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:20:24.81 +69:02:06.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.72, MAG_FAINT_SEARCH_LIMIT=13.70)GAIADR2_OUTPUT=# 4.191 541146573421830144 050.10096953861 +69.03443811154 13.4068 12.7800 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.191#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133075_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133075_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:11:06.53 +73:01:06.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.75, MAG_FAINT_SEARCH_LIMIT=13.73)GAIADR2_OUTPUT=# 5.239 544310005812169472 047.77247928522 +73.01798617756 13.1394 12.4100 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.239#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133076_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133076_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133078_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133078_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:07:42.83 +72:41:44.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 0.904 544204968092589952 046.92871587127 +72.69542766433 13.1355 12.4879 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.904#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133082_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133082_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133086_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133086_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:15:38.34 +72:08:11.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.49, MAG_FAINT_SEARCH_LIMIT=13.47)GAIADR2_OUTPUT=# 0.794 543943868440687872 048.90960934964 +72.13628374211 13.0840 12.4080 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.794#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133091_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133091_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133092_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133092_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:13:06.44 +71:38:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.60, MAG_FAINT_SEARCH_LIMIT=13.58)GAIADR2_OUTPUT=# 0.893 543892225754092672 048.27742994169 +71.63371757802 13.0406 12.4071 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.893#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133095_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133095_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:09:21.67 +72:02:58.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.50, MAG_FAINT_SEARCH_LIMIT=13.48)GAIADR2_OUTPUT=# 5.013 544106561802438272 047.33600925288 +72.04922247502 13.2007 12.5563 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.013#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133101_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133101_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133104_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133104_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:17:53.08 +71:03:27.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 2.823 543065289931320448 049.46881415020 +71.05787285418 13.1624 12.3402 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.823#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133107_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133107_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (12.0") between the two second-epoch detections
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Considering the candidate 133110_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133110_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133111_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133111_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 133112_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133112_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133113_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133113_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133114_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133114_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133115_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133115_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133118_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133118_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:12:36.55 +72:30:53.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.13, MAG_FAINT_SEARCH_LIMIT=13.11)GAIADR2_OUTPUT=# 1.341 544155043393141504 048.15303558370 +72.51464635444 12.7076 12.0773 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.341#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133119_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133119_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133128_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133128_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:21:20.59 +72:14:55.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.25, MAG_FAINT_SEARCH_LIMIT=13.23)GAIADR2_OUTPUT=# 4.427 543983141621407360 050.33931421997 +72.24943213116 12.7802 12.1622 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.427#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133132_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133132_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:22:38.89 +73:43:38.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 3.660 544733420868613248 050.66543968723 +73.72768942289 12.8749 12.2779 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.660#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133134_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133134_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133135_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133135_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133136_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133136_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:07:59.30 +72:35:32.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.22, MAG_FAINT_SEARCH_LIMIT=13.20)GAIADR2_OUTPUT=# 4.281 544200466966891136 047.00105725508 +72.59244904343 12.7544 12.1714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.281#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133137_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133137_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:48:57.11 +65:32:22.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.19, MAG_FAINT_SEARCH_LIMIT=13.17)GAIADR2_OUTPUT=# 1.819 488357027307740544 057.23722571476 +65.53912352695 13.0320 11.8593 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.819#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133141_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133141_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133146_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133146_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133151_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133151_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133153_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133153_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133160_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133160_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:18:02.36 +73:15:59.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.88, MAG_FAINT_SEARCH_LIMIT=12.86)GAIADR2_OUTPUT=# 5.785 544293066461248512 049.51486855575 +73.26713781224 12.3758 11.7596 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.785#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133170_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133170_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:25:48.79 +73:55:40.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.59, MAG_FAINT_SEARCH_LIMIT=12.57)GAIADR2_OUTPUT=# 3.163 544713350484492160 051.45049346861 +73.92736326432 12.3953 11.8454 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.163#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133171_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133171_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:09:36.37 +73:39:59.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.62, MAG_FAINT_SEARCH_LIMIT=12.60)GAIADR2_OUTPUT=# 5.458 547357332351238656 047.40675144048 +73.66697332038 12.3151 11.7300 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.458#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133173_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133173_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:36:33.61 +66:04:19.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.75, MAG_FAINT_SEARCH_LIMIT=12.73)GAIADR2_OUTPUT=# 3.381 491619308369939328 054.13796996378 +66.07155267326 12.5861 11.5358 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.381#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133174_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133174_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:16:56.29 +73:32:46.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.50, MAG_FAINT_SEARCH_LIMIT=12.48)GAIADR2_OUTPUT=# 2.870 544352573231049984 049.23172921709 +73.54628446708 12.1004 11.4207 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.870#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133175_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133175_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:15:05.98 +70:35:19.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.51, MAG_FAINT_SEARCH_LIMIT=12.49)GAIADR2_OUTPUT=# 2.625 541538441940524160 048.77694708219 +70.58910948363 12.3033 11.7714 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.625#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133178_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133178_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133179_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133179_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:20:42.95 +69:26:32.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.18, MAG_FAINT_SEARCH_LIMIT=12.16)GAIADR2_OUTPUT=# 2.065 541193611903567232 050.18027212905 +69.44275751907 12.0022 11.3346 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.065#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133180_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133180_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:11:51.70 +73:33:29.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.19, MAG_FAINT_SEARCH_LIMIT=12.17)GAIADR2_OUTPUT=# 5.126 547363757623605248 047.97037810001 +73.55851354013 11.8966 11.3302 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.126#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133181_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133181_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
Rejecting candidate due to large distance (16.7") between the two second-epoch detections
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Considering the candidate 133182_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133182_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133183_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133183_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133186_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133186_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:09:27.32 +72:56:37.0 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=10.74, MAG_FAINT_SEARCH_LIMIT=11.72)
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Considering the candidate 133187_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133187_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:10:00.25 +71:57:10.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.66, MAG_FAINT_SEARCH_LIMIT=11.64)GAIADR2_OUTPUT=# 3.925 544102198115675008 047.49789313698 +71.95229085482 11.1685 10.4829 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.925#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133188_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133188_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:12:30.02 +73:14:00.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.63, MAG_FAINT_SEARCH_LIMIT=11.61)GAIADR2_OUTPUT=# 5.070 544329419064311296 048.12027919604 +73.23330463762 11.3068 10.7679 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.070#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133189_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133189_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:16:14.08 +70:14:13.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.58, MAG_FAINT_SEARCH_LIMIT=11.56)GAIADR2_OUTPUT=# 2.709 541479858585212672 049.06034481205 +70.23754968270 11.3809 10.7618 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.709#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133190_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133190_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:04:15.85 +73:20:56.5 in APASS (TIMEOUTCOMMAND_GAIA_VIZIER=#timeout 40 #, MAG_MEAN=10.53, MAG_FAINT_SEARCH_LIMIT=11.51)
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Considering the candidate 133252_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133252_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133645_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 133645_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:42:42.90 +64:44:19.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=10.73, MAG_FAINT_SEARCH_LIMIT=11.71)GAIADR2_OUTPUT=# 4.007 488212201011316480 055.67736897839 +64.73766679550 11.6343 10.6963 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#4.007#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133730_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133730_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133786_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133786_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133810_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133810_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133897_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133897_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 133960_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 133960_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 134220_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 134220_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 134307_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 134307_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 134372_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 134372_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 134427_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 134427_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 134556_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 134556_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 134645_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 134645_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 135184_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 135184_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:17:16.51 +66:57:58.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.39, MAG_FAINT_SEARCH_LIMIT=13.37)GAIADR2_OUTPUT=# 3.326 489701042833419648 064.31682306768 +66.96573963736 12.3157 10.3326 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.326#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135231_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 135231_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 135324_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 135324_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 135331_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 135331_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:59:41.04 +70:26:56.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 1.001 494992098945297152 059.92047422755 +70.44872909789 13.4024 12.5394 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.001#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135334_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 135334_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 135345_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 135345_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 135478_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 135478_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 135479_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 135479_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:20:28.37 +65:07:06.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 135546_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 135546_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 06:20:44.64 +72:07:05.2 in the exclusion list exclusion_list.txt ****
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Considering the candidate 135583_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 135583_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 135614_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 135614_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 135725_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 135725_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 135746_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 135746_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 135850_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 135850_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 135944_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 135944_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 136003_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136003_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 136005_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136005_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136075_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 136075_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:35:40.86 +64:38:21.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.82, MAG_FAINT_SEARCH_LIMIT=13.80)GAIADR2_OUTPUT=# 5.553 488383827904758272 053.91769922421 +64.63827235038 13.5273 12.5359 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.553#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 136111_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136111_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 136152_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 136152_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 05:09:35.52 +64:54:04.7 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 136248_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136248_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 136259_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136259_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 136280_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136280_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 136284_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136284_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 136305_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136305_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136325_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136325_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136327_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136327_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136470_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136470_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136473_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136473_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
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Considering the candidate 136532_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136532_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136599_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136599_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136693_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136693_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136796_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136796_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136833_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136833_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136845_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136845_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136853_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136853_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136867_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136867_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136868_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136868_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136876_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136876_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136881_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136881_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136892_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 136892_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:03:28.38 +69:29:38.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.099 494039750077042048 060.86975667211 +69.49416448411 14.3622 13.4719 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.099#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136895_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 136895_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:26:19.63 +64:53:32.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.29, MAG_FAINT_SEARCH_LIMIT=14.27)GAIADR2_OUTPUT=# 1.898 477049787167366656 066.58223817107 +64.89184127694 14.0534 12.9466 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.898#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136943_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136943_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136981_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136981_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136985_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136985_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136995_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 136995_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137012_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 137012_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:30:02.81 +66:07:14.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.34, MAG_FAINT_SEARCH_LIMIT=14.32)GAIADR2_OUTPUT=# 2.047 477362082828879360 067.51257116406 +66.12024586113 14.2693 13.3151 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.047#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137044_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137044_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137048_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 137048_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:22:21.31 +65:57:34.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.46, MAG_FAINT_SEARCH_LIMIT=14.44)GAIADR2_OUTPUT=# 2.204 489352050971194368 065.58970917263 +65.95898736608 12.9446 11.3719 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.204#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137088_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137088_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137145_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137145_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137168_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137168_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137187_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137187_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137212_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137212_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137239_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137239_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137265_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137265_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137306_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137306_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137320_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137320_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137322_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137322_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137330_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137330_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137353_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137353_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137357_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137357_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137365_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137365_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137366_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137366_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137371_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137371_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137384_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137384_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137406_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137406_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137409_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137409_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137417_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137417_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137418_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137418_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137423_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137423_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137424_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137424_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137434_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137434_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137437_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 137437_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:21:55.32 +65:02:54.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 2.478 477163139942578816 065.48099096975 +65.04778807924 14.3731 13.2667 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.478#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137472_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137472_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137485_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137485_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137503_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137503_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137505_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137505_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137524_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137524_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137543_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137543_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137545_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137545_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137550_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137550_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137560_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137560_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137572_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 137572_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 04:17:43.74 +66:07:37.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.61, MAG_FAINT_SEARCH_LIMIT=14.59)GAIADR2_OUTPUT=# 3.224 489335867533606400 064.43439288130 +66.12683186600 14.5612 13.4269 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#3.224#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137575_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137575_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137604_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137604_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137607_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 137607_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 03:56:22.27 +69:50:16.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.57, MAG_FAINT_SEARCH_LIMIT=14.55)GAIADR2_OUTPUT=# 1.240 494118055920331392 059.09348636704 +69.83755807704 14.4674 13.5681 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.240#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137609_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137609_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137635_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137635_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137650_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137650_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137652_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137652_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137658_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137658_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137665_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137665_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137682_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137682_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137689_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137689_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137694_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
The candidate 137694_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101 did not pass the final checks
**** FOUND 06:04:17.01 +71:17:02.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.70, MAG_FAINT_SEARCH_LIMIT=14.68)GAIADR2_OUTPUT=# 0.237 1107724056220046720 091.07101062912 +71.28386729106 14.5166 13.3707 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.237#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 137720_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 137720_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90043_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 90043_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 02641_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 02641_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 43023_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
Preparing report for the candidate 43023_fd_Cam-06-Q2b1x1_2026-03-19_22-32-08_20.00sec_-14.90C_LIGHT_0101
make_report_in_HTML.sh Phase 2 (HTML assembly): 30s
make_report_in_HTML.sh TOTAL: 332s
Prepared the HTML report for the field Cam-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
06:23:58.24 +72:38:04.4
04:59:41.46 +67:23:00.4
05:05:09.09 +66:23:19.0
04:49:03.90 +69:07:43.6
05:07:51.50 +65:22:30.5
05:02:11.36 +66:07:00.4
05:03:35.97 +68:40:13.4
05:55:54.35 +66:08:23.3
05:11:38.57 +64:54:35.6
05:11:48.71 +66:41:11.0
05:25:12.19 +66:12:19.7
03:56:03.26 +69:57:42.2
04:24:13.44 +70:35:39.4
04:30:36.89 +74:25:32.2
06:03:51.51 +70:17:17.6
05:07:26.76 +73:55:10.8
05:22:24.96 +66:19:03.7
05:58:17.58 +67:53:45.5
04:34:47.55 +66:05:05.8
05:03:27.18 +73:34:55.3
03:12:38.28 +72:39:11.6
03:18:08.68 +71:39:25.8
05:44:28.49 +64:32:52.2
04:11:33.37 +65:34:23.2
03:17:10.56 +69:54:48.5
03:10:42.63 +73:30:53.5
04:32:28.46 +67:14:27.4
03:22:24.94 +73:47:02.3
03:46:01.35 +69:29:05.8
04:54:50.39 +66:57:16.6
05:02:53.69 +65:01:14.4
04:32:07.11 +69:05:37.1
04:02:19.67 +70:42:08.3
05:12:59.98 +68:41:28.7
03:13:13.23 +72:32:45.4
03:15:24.46 +73:35:27.6
03:08:09.62 +72:20:39.1
04:22:14.21 +65:32:26.1
03:07:49.50 +72:26:25.5
03:12:19.68 +71:19:44.4
03:08:28.72 +72:22:00.5
03:13:32.43 +71:53:25.2
03:15:15.25 +70:34:15.1
04:20:32.42 +67:29:55.0
04:36:17.78 +72:45:20.9
03:14:45.18 +72:01:17.1
03:08:57.58 +72:54:01.9
03:14:47.53 +73:15:58.9
04:05:44.41 +69:16:50.2
03:45:58.45 +68:00:22.8
03:10:42.06 +73:20:48.1
04:30:48.67 +64:51:50.5
03:53:34.78 +64:50:56.9
05:33:26.98 +65:17:16.9
03:43:49.03 +64:45:07.2
04:00:27.78 +68:34:39.7
04:29:51.32 +65:59:10.2
04:42:14.52 +69:04:10.6
04:18:40.67 +74:39:11.6
04:59:39.30 +71:29:48.0
05:46:27.89 +68:07:41.2
04:18:00.86 +71:13:59.0
04:57:37.99 +70:38:35.3
05:17:15.95 +73:34:57.9
04:00:50.26 +67:35:24.1
04:27:04.11 +67:43:40.4
04:29:19.00 +69:15:33.7
05:55:20.52 +64:07:13.5
04:50:16.69 +72:56:19.2
04:50:31.26 +70:07:14.5
03:57:23.35 +71:25:00.4
04:50:22.42 +72:53:50.5
05:53:03.71 +64:13:58.4
05:21:43.12 +66:47:48.5
04:16:56.09 +69:09:47.9
04:55:33.01 +66:54:52.5
04:29:19.56 +69:31:53.2
04:56:30.86 +72:51:34.2
04:20:01.12 +68:13:26.2
04:45:55.16 +68:04:57.6
05:17:22.73 +71:24:55.0
04:14:47.99 +68:29:38.1
05:29:55.17 +74:30:44.9
05:03:33.84 +65:44:44.7
05:24:01.23 +71:37:20.2
06:05:07.94 +67:40:12.8
05:15:56.81 +70:34:25.3
04:38:34.60 +65:24:55.1
05:07:59.82 +65:47:22.8
05:39:11.34 +68:47:03.4
04:59:15.34 +65:54:52.3
05:01:54.54 +71:44:42.3
05:36:09.32 +69:59:53.6
04:58:10.25 +65:24:26.3
04:24:34.32 +67:41:09.7
05:06:10.92 +64:52:32.5
05:01:07.01 +70:03:24.2
06:01:10.95 +71:55:17.3
04:32:40.04 +65:00:00.0
05:41:41.12 +70:56:51.2
05:11:19.27 +72:08:07.6
04:02:25.59 +66:01:46.0
04:51:35.87 +65:30:23.6
04:43:20.69 +72:22:21.8
04:32:18.16 +66:04:29.9
05:20:32.39 +65:19:26.7
04:41:55.49 +65:26:14.8
05:48:13.93 +67:04:45.2
04:02:09.32 +70:45:37.7
04:41:09.33 +67:50:57.0
04:12:01.89 +69:32:11.6
04:06:53.12 +65:28:30.0
05:20:36.05 +66:22:28.4
04:39:49.20 +67:53:55.8
05:54:24.56 +67:33:40.0
04:56:17.91 +70:32:23.5
04:40:44.63 +71:13:49.0
05:19:50.18 +70:16:36.3
05:46:48.60 +66:28:28.0
06:02:49.55 +66:59:08.9
04:35:53.88 +65:39:42.0
06:09:07.02 +72:22:40.1
05:06:50.26 +64:51:24.5
04:05:46.24 +69:03:16.9
05:25:27.13 +68:03:13.8
04:54:44.70 +65:04:14.9
05:00:53.03 +64:54:36.1
04:52:46.89 +67:49:23.1
05:48:20.98 +70:52:48.7
04:15:09.85 +69:56:55.4
04:13:11.73 +67:46:21.7
04:25:21.76 +65:57:39.6
06:07:07.42 +71:41:37.3
03:58:05.38 +65:01:43.4
05:11:49.87 +65:47:00.4
05:06:00.80 +66:58:52.0
05:19:54.25 +71:34:18.4
04:29:42.40 +65:27:15.7
05:27:50.85 +66:14:55.8
04:25:57.70 +74:11:24.3
04:42:25.97 +67:11:09.6
04:42:27.84 +68:36:52.3
04:51:07.98 +69:25:24.9
03:57:36.41 +67:28:34.5
05:31:40.78 +70:19:44.6
05:45:20.27 +72:47:19.3
03:28:21.89 +70:57:01.0
04:05:39.55 +66:19:58.3
########### Completed Cam-06-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
04:59:41.46 +67:23:00.4
05:05:09.09 +66:23:19.0
04:49:03.90 +69:07:43.6
05:07:51.50 +65:22:30.5
05:02:11.36 +66:07:00.4
05:03:35.97 +68:40:13.4
05:55:54.35 +66:08:23.3
05:11:38.57 +64:54:35.6
05:11:48.71 +66:41:11.0
05:25:12.19 +66:12:19.7
03:56:03.26 +69:57:42.2
04:24:13.44 +70:35:39.4
04:30:36.89 +74:25:32.2
06:03:51.51 +70:17:17.6
05:07:26.76 +73:55:10.8
05:22:24.96 +66:19:03.7
05:58:17.58 +67:53:45.5
04:34:47.55 +66:05:05.8
05:03:27.18 +73:34:55.3
03:12:38.28 +72:39:11.6
03:18:08.68 +71:39:25.8
05:44:28.49 +64:32:52.2
04:11:33.37 +65:34:23.2
03:17:10.56 +69:54:48.5
03:10:42.63 +73:30:53.5
04:32:28.46 +67:14:27.4
03:22:24.94 +73:47:02.3
03:46:01.35 +69:29:05.8
04:54:50.39 +66:57:16.6
05:02:53.69 +65:01:14.4
04:32:07.11 +69:05:37.1
04:02:19.67 +70:42:08.3
05:12:59.98 +68:41:28.7
03:13:13.23 +72:32:45.4
03:15:24.46 +73:35:27.6
03:08:09.62 +72:20:39.1
04:22:14.21 +65:32:26.1
03:07:49.50 +72:26:25.5
03:12:19.68 +71:19:44.4
03:08:28.72 +72:22:00.5
03:13:32.43 +71:53:25.2
03:15:15.25 +70:34:15.1
04:20:32.42 +67:29:55.0
04:36:17.78 +72:45:20.9
03:14:45.18 +72:01:17.1
03:08:57.58 +72:54:01.9
03:14:47.53 +73:15:58.9
04:05:44.41 +69:16:50.2
03:45:58.45 +68:00:22.8
03:10:42.06 +73:20:48.1
04:30:48.67 +64:51:50.5
03:53:34.78 +64:50:56.9
05:33:26.98 +65:17:16.9
03:43:49.03 +64:45:07.2
04:00:27.78 +68:34:39.7
04:29:51.32 +65:59:10.2
04:42:14.52 +69:04:10.6
04:18:40.67 +74:39:11.6
04:59:39.30 +71:29:48.0
05:46:27.89 +68:07:41.2
04:18:00.86 +71:13:59.0
04:57:37.99 +70:38:35.3
05:17:15.95 +73:34:57.9
04:00:50.26 +67:35:24.1
04:27:04.11 +67:43:40.4
04:29:19.00 +69:15:33.7
05:55:20.52 +64:07:13.5
04:50:16.69 +72:56:19.2
04:50:31.26 +70:07:14.5
03:57:23.35 +71:25:00.4
04:50:22.42 +72:53:50.5
05:53:03.71 +64:13:58.4
05:21:43.12 +66:47:48.5
04:16:56.09 +69:09:47.9
04:55:33.01 +66:54:52.5
04:29:19.56 +69:31:53.2
04:56:30.86 +72:51:34.2
04:20:01.12 +68:13:26.2
04:45:55.16 +68:04:57.6
05:17:22.73 +71:24:55.0
04:14:47.99 +68:29:38.1
05:29:55.17 +74:30:44.9
05:03:33.84 +65:44:44.7
05:24:01.23 +71:37:20.2
06:05:07.94 +67:40:12.8
05:15:56.81 +70:34:25.3
04:38:34.60 +65:24:55.1
05:07:59.82 +65:47:22.8
05:39:11.34 +68:47:03.4
04:59:15.34 +65:54:52.3
05:01:54.54 +71:44:42.3
05:36:09.32 +69:59:53.6
04:58:10.25 +65:24:26.3
04:24:34.32 +67:41:09.7
05:06:10.92 +64:52:32.5
05:01:07.01 +70:03:24.2
06:01:10.95 +71:55:17.3
04:32:40.04 +65:00:00.0
05:41:41.12 +70:56:51.2
05:11:19.27 +72:08:07.6
04:02:25.59 +66:01:46.0
04:51:35.87 +65:30:23.6
04:43:20.69 +72:22:21.8
04:32:18.16 +66:04:29.9
05:20:32.39 +65:19:26.7
04:41:55.49 +65:26:14.8
05:48:13.93 +67:04:45.2
04:02:09.32 +70:45:37.7
04:41:09.33 +67:50:57.0
04:12:01.89 +69:32:11.6
04:06:53.12 +65:28:30.0
05:20:36.05 +66:22:28.4
04:39:49.20 +67:53:55.8
05:54:24.56 +67:33:40.0
04:56:17.91 +70:32:23.5
04:40:44.63 +71:13:49.0
05:19:50.18 +70:16:36.3
05:46:48.60 +66:28:28.0
06:02:49.55 +66:59:08.9
04:35:53.88 +65:39:42.0
06:09:07.02 +72:22:40.1
05:06:50.26 +64:51:24.5
04:05:46.24 +69:03:16.9
05:25:27.13 +68:03:13.8
04:54:44.70 +65:04:14.9
05:00:53.03 +64:54:36.1
04:52:46.89 +67:49:23.1
05:48:20.98 +70:52:48.7
04:15:09.85 +69:56:55.4
04:13:11.73 +67:46:21.7
04:25:21.76 +65:57:39.6
06:07:07.42 +71:41:37.3
03:58:05.38 +65:01:43.4
05:11:49.87 +65:47:00.4
05:06:00.80 +66:58:52.0
05:19:54.25 +71:34:18.4
04:29:42.40 +65:27:15.7
05:27:50.85 +66:14:55.8
04:25:57.70 +74:11:24.3
04:42:25.97 +67:11:09.6
04:42:27.84 +68:36:52.3
04:51:07.98 +69:25:24.9
03:57:36.41 +67:28:34.5
05:31:40.78 +70:19:44.6
05:45:20.27 +72:47:19.3
04:05:39.55 +66:19:58.3
06:23:58.24 +72:38:04.4
03:28:21.89 +70:57:01.0
###################################################################################
04:59:41.46 +67:23:00.4 -- not an asteroid (will add it to exclusion list)
05:05:09.09 +66:23:19.0 -- not an asteroid (will add it to exclusion list)
04:49:03.90 +69:07:43.6 -- not an asteroid (will add it to exclusion list)
05:07:51.50 +65:22:30.5 -- not an asteroid (will add it to exclusion list)
05:02:11.36 +66:07:00.4 -- not an asteroid (will add it to exclusion list)
05:03:35.97 +68:40:13.4 -- not an asteroid (will add it to exclusion list)
05:55:54.35 +66:08:23.3 -- not an asteroid (will add it to exclusion list)
05:11:38.57 +64:54:35.6 -- not an asteroid (will add it to exclusion list)
05:11:48.71 +66:41:11.0 -- not an asteroid (will add it to exclusion list)
05:25:12.19 +66:12:19.7 -- not an asteroid (will add it to exclusion list)
03:56:03.26 +69:57:42.2 -- not an asteroid (will add it to exclusion list)
04:24:13.44 +70:35:39.4 -- not an asteroid (will add it to exclusion list)
04:30:36.89 +74:25:32.2 -- not an asteroid (will add it to exclusion list)
06:03:51.51 +70:17:17.6 -- not an asteroid (will add it to exclusion list)
05:07:26.76 +73:55:10.8 -- not an asteroid (will add it to exclusion list)
05:22:24.96 +66:19:03.7 -- not an asteroid (will add it to exclusion list)
05:58:17.58 +67:53:45.5 -- not an asteroid (will add it to exclusion list)
04:34:47.55 +66:05:05.8 -- not an asteroid (will add it to exclusion list)
05:03:27.18 +73:34:55.3 -- not an asteroid (will add it to exclusion list)
03:12:38.28 +72:39:11.6 -- not an asteroid (will add it to exclusion list)
03:18:08.68 +71:39:25.8 -- not an asteroid (will add it to exclusion list)
05:44:28.49 +64:32:52.2 -- not an asteroid (will add it to exclusion list)
04:11:33.37 +65:34:23.2 -- not an asteroid (will add it to exclusion list)
03:17:10.56 +69:54:48.5 -- not an asteroid (will add it to exclusion list)
03:10:42.63 +73:30:53.5 -- not an asteroid (will add it to exclusion list)
04:32:28.46 +67:14:27.4 -- not an asteroid (will add it to exclusion list)
03:22:24.94 +73:47:02.3 -- not an asteroid (will add it to exclusion list)
03:46:01.35 +69:29:05.8 -- not an asteroid (will add it to exclusion list)
04:54:50.39 +66:57:16.6 -- not an asteroid (will add it to exclusion list)
05:02:53.69 +65:01:14.4 -- not an asteroid (will add it to exclusion list)
04:32:07.11 +69:05:37.1 -- not an asteroid (will add it to exclusion list)
04:02:19.67 +70:42:08.3 -- not an asteroid (will add it to exclusion list)
05:12:59.98 +68:41:28.7 -- not an asteroid (will add it to exclusion list)
03:13:13.23 +72:32:45.4 -- not an asteroid (will add it to exclusion list)
03:15:24.46 +73:35:27.6 -- not an asteroid (will add it to exclusion list)
03:08:09.62 +72:20:39.1 -- not an asteroid (will add it to exclusion list)
04:22:14.21 +65:32:26.1 -- not an asteroid (will add it to exclusion list)
03:07:49.50 +72:26:25.5 -- not an asteroid (will add it to exclusion list)
03:12:19.68 +71:19:44.4 -- not an asteroid (will add it to exclusion list)
03:08:28.72 +72:22:00.5 -- not an asteroid (will add it to exclusion list)
03:13:32.43 +71:53:25.2 -- not an asteroid (will add it to exclusion list)
03:15:15.25 +70:34:15.1 -- not an asteroid (will add it to exclusion list)
04:20:32.42 +67:29:55.0 -- not an asteroid (will add it to exclusion list)
04:36:17.78 +72:45:20.9 -- not an asteroid (will add it to exclusion list)
03:14:45.18 +72:01:17.1 -- not an asteroid (will add it to exclusion list)
03:08:57.58 +72:54:01.9 -- not an asteroid (will add it to exclusion list)
03:14:47.53 +73:15:58.9 -- not an asteroid (will add it to exclusion list)
04:05:44.41 +69:16:50.2 -- not an asteroid (will add it to exclusion list)
03:45:58.45 +68:00:22.8 -- not an asteroid (will add it to exclusion list)
03:10:42.06 +73:20:48.1 -- not an asteroid (will add it to exclusion list)
04:30:48.67 +64:51:50.5 -- not an asteroid (will add it to exclusion list)
03:53:34.78 +64:50:56.9 -- not an asteroid (will add it to exclusion list)
05:33:26.98 +65:17:16.9 -- not an asteroid (will add it to exclusion list)
03:43:49.03 +64:45:07.2 -- not an asteroid (will add it to exclusion list)
04:00:27.78 +68:34:39.7 -- not an asteroid (will add it to exclusion list)
04:29:51.32 +65:59:10.2 -- not an asteroid (will add it to exclusion list)
04:42:14.52 +69:04:10.6 -- not an asteroid (will add it to exclusion list)
04:18:40.67 +74:39:11.6 -- not an asteroid (will add it to exclusion list)
04:59:39.30 +71:29:48.0 -- not an asteroid (will add it to exclusion list)
05:46:27.89 +68:07:41.2 -- not an asteroid (will add it to exclusion list)
04:18:00.86 +71:13:59.0 -- not an asteroid (will add it to exclusion list)
04:57:37.99 +70:38:35.3 -- not an asteroid (will add it to exclusion list)
05:17:15.95 +73:34:57.9 -- not an asteroid (will add it to exclusion list)
04:00:50.26 +67:35:24.1 -- not an asteroid (will add it to exclusion list)
04:27:04.11 +67:43:40.4 -- not an asteroid (will add it to exclusion list)
04:29:19.00 +69:15:33.7 -- not an asteroid (will add it to exclusion list)
05:55:20.52 +64:07:13.5 -- not an asteroid (will add it to exclusion list)
04:50:16.69 +72:56:19.2 -- not an asteroid (will add it to exclusion list)
04:50:31.26 +70:07:14.5 -- not an asteroid (will add it to exclusion list)
03:57:23.35 +71:25:00.4 -- not an asteroid (will add it to exclusion list)
04:50:22.42 +72:53:50.5 -- not an asteroid (will add it to exclusion list)
05:53:03.71 +64:13:58.4 -- not an asteroid (will add it to exclusion list)
05:21:43.12 +66:47:48.5 -- not an asteroid (will add it to exclusion list)
04:16:56.09 +69:09:47.9 -- not an asteroid (will add it to exclusion list)
04:55:33.01 +66:54:52.5 -- not an asteroid (will add it to exclusion list)
04:29:19.56 +69:31:53.2 -- not an asteroid (will add it to exclusion list)
04:56:30.86 +72:51:34.2 -- not an asteroid (will add it to exclusion list)
04:20:01.12 +68:13:26.2 -- not an asteroid (will add it to exclusion list)
04:45:55.16 +68:04:57.6 -- not an asteroid (will add it to exclusion list)
05:17:22.73 +71:24:55.0 -- not an asteroid (will add it to exclusion list)
04:14:47.99 +68:29:38.1 -- not an asteroid (will add it to exclusion list)
05:29:55.17 +74:30:44.9 -- not an asteroid (will add it to exclusion list)
05:03:33.84 +65:44:44.7 -- not an asteroid (will add it to exclusion list)
05:24:01.23 +71:37:20.2 -- not an asteroid (will add it to exclusion list)
06:05:07.94 +67:40:12.8 -- not an asteroid (will add it to exclusion list)
05:15:56.81 +70:34:25.3 -- not an asteroid (will add it to exclusion list)
04:38:34.60 +65:24:55.1 -- not an asteroid (will add it to exclusion list)
05:07:59.82 +65:47:22.8 -- not an asteroid (will add it to exclusion list)
05:39:11.34 +68:47:03.4 -- not an asteroid (will add it to exclusion list)
04:59:15.34 +65:54:52.3 -- not an asteroid (will add it to exclusion list)
05:01:54.54 +71:44:42.3 -- not an asteroid (will add it to exclusion list)
05:36:09.32 +69:59:53.6 -- not an asteroid (will add it to exclusion list)
04:58:10.25 +65:24:26.3 -- not an asteroid (will add it to exclusion list)
04:24:34.32 +67:41:09.7 -- not an asteroid (will add it to exclusion list)
05:06:10.92 +64:52:32.5 -- not an asteroid (will add it to exclusion list)
05:01:07.01 +70:03:24.2 -- not an asteroid (will add it to exclusion list)
06:01:10.95 +71:55:17.3 -- not an asteroid (will add it to exclusion list)
04:32:40.04 +65:00:00.0 -- not an asteroid (will add it to exclusion list)
05:41:41.12 +70:56:51.2 -- not an asteroid (will add it to exclusion list)
05:11:19.27 +72:08:07.6 -- not an asteroid (will add it to exclusion list)
04:02:25.59 +66:01:46.0 -- not an asteroid (will add it to exclusion list)
04:51:35.87 +65:30:23.6 -- not an asteroid (will add it to exclusion list)
04:43:20.69 +72:22:21.8 -- not an asteroid (will add it to exclusion list)
04:32:18.16 +66:04:29.9 -- not an asteroid (will add it to exclusion list)
05:20:32.39 +65:19:26.7 -- not an asteroid (will add it to exclusion list)
04:41:55.49 +65:26:14.8 -- not an asteroid (will add it to exclusion list)
05:48:13.93 +67:04:45.2 -- not an asteroid (will add it to exclusion list)
04:02:09.32 +70:45:37.7 -- not an asteroid (will add it to exclusion list)
04:41:09.33 +67:50:57.0 -- not an asteroid (will add it to exclusion list)
04:12:01.89 +69:32:11.6 -- not an asteroid (will add it to exclusion list)
04:06:53.12 +65:28:30.0 -- not an asteroid (will add it to exclusion list)
05:20:36.05 +66:22:28.4 -- not an asteroid (will add it to exclusion list)
04:39:49.20 +67:53:55.8 -- not an asteroid (will add it to exclusion list)
05:54:24.56 +67:33:40.0 -- not an asteroid (will add it to exclusion list)
04:56:17.91 +70:32:23.5 -- not an asteroid (will add it to exclusion list)
04:40:44.63 +71:13:49.0 -- not an asteroid (will add it to exclusion list)
05:19:50.18 +70:16:36.3 -- not an asteroid (will add it to exclusion list)
05:46:48.60 +66:28:28.0 -- not an asteroid (will add it to exclusion list)
06:02:49.55 +66:59:08.9 -- not an asteroid (will add it to exclusion list)
04:35:53.88 +65:39:42.0 -- not an asteroid (will add it to exclusion list)
06:09:07.02 +72:22:40.1 -- not an asteroid (will add it to exclusion list)
05:06:50.26 +64:51:24.5 -- not an asteroid (will add it to exclusion list)
04:05:46.24 +69:03:16.9 -- not an asteroid (will add it to exclusion list)
05:25:27.13 +68:03:13.8 -- not an asteroid (will add it to exclusion list)
04:54:44.70 +65:04:14.9 -- not an asteroid (will add it to exclusion list)
05:00:53.03 +64:54:36.1 -- not an asteroid (will add it to exclusion list)
04:52:46.89 +67:49:23.1 -- not an asteroid (will add it to exclusion list)
05:48:20.98 +70:52:48.7 -- not an asteroid (will add it to exclusion list)
04:15:09.85 +69:56:55.4 -- not an asteroid (will add it to exclusion list)
04:13:11.73 +67:46:21.7 -- not an asteroid (will add it to exclusion list)
04:25:21.76 +65:57:39.6 -- not an asteroid (will add it to exclusion list)
06:07:07.42 +71:41:37.3 -- not an asteroid (will add it to exclusion list)
03:58:05.38 +65:01:43.4 -- not an asteroid (will add it to exclusion list)
05:11:49.87 +65:47:00.4 -- not an asteroid (will add it to exclusion list)
05:06:00.80 +66:58:52.0 -- not an asteroid (will add it to exclusion list)
05:19:54.25 +71:34:18.4 -- not an asteroid (will add it to exclusion list)
04:29:42.40 +65:27:15.7 -- not an asteroid (will add it to exclusion list)
05:27:50.85 +66:14:55.8 -- not an asteroid (will add it to exclusion list)
04:25:57.70 +74:11:24.3 -- not an asteroid (will add it to exclusion list)
04:42:25.97 +67:11:09.6 -- not an asteroid (will add it to exclusion list)
04:42:27.84 +68:36:52.3 -- not an asteroid (will add it to exclusion list)
04:51:07.98 +69:25:24.9 -- not an asteroid (will add it to exclusion list)
03:57:36.41 +67:28:34.5 -- not an asteroid (will add it to exclusion list)
05:31:40.78 +70:19:44.6 -- not an asteroid (will add it to exclusion list)
05:45:20.27 +72:47:19.3 -- not an asteroid (will add it to exclusion list)
04:05:39.55 +66:19:58.3 -- not an asteroid (will add it to exclusion list)
06:23:58.24 +72:38:04.4 -- not an asteroid (will add it to exclusion list)
03:28:21.89 +70:57:01.0 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
03:07:49.50 +72:26:25.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:08:09.62 +72:20:39.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:08:28.72 +72:22:00.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:08:57.58 +72:54:01.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:10:42.06 +73:20:48.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:10:42.63 +73:30:53.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:12:19.68 +71:19:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:12:38.28 +72:39:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:13:13.23 +72:32:45.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:13:32.43 +71:53:25.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:14:45.18 +72:01:17.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:14:47.53 +73:15:58.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:15:15.25 +70:34:15.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:15:24.46 +73:35:27.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:17:10.56 +69:54:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:18:08.68 +71:39:25.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:22:24.94 +73:47:02.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:28:21.89 +70:57:01.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:49.03 +64:45:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:58.45 +68:00:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:01.35 +69:29:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:34.78 +64:50:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:56:03.26 +69:57:42.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:57:23.35 +71:25:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:57:36.41 +67:28:34.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:58:05.38 +65:01:43.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:00:27.78 +68:34:39.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:00:50.26 +67:35:24.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:02:09.32 +70:45:37.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:02:19.67 +70:42:08.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:02:25.59 +66:01:46.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:39.55 +66:19:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:44.41 +69:16:50.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:46.24 +69:03:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:06:53.12 +65:28:30.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:11:33.37 +65:34:23.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:12:01.89 +69:32:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:13:11.73 +67:46:21.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:14:47.99 +68:29:38.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:15:09.85 +69:56:55.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:16:56.09 +69:09:47.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:18:00.86 +71:13:59.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:18:40.67 +74:39:11.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:20:01.12 +68:13:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:20:32.42 +67:29:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:22:14.21 +65:32:26.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:13.44 +70:35:39.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:34.32 +67:41:09.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:21.76 +65:57:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:57.70 +74:11:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:27:04.11 +67:43:40.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:29:19.00 +69:15:33.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:29:19.56 +69:31:53.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:29:42.40 +65:27:15.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:29:51.32 +65:59:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:30:36.89 +74:25:32.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:30:48.67 +64:51:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:07.11 +69:05:37.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:18.16 +66:04:29.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:28.46 +67:14:27.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:40.04 +65:00:00.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:34:47.55 +66:05:05.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:35:53.88 +65:39:42.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:36:17.78 +72:45:20.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:38:34.60 +65:24:55.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:39:49.20 +67:53:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:40:44.63 +71:13:49.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:41:09.33 +67:50:57.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:41:55.49 +65:26:14.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:42:14.52 +69:04:10.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:42:25.97 +67:11:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:42:27.84 +68:36:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:43:20.69 +72:22:21.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:45:55.16 +68:04:57.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:49:03.90 +69:07:43.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:50:16.69 +72:56:19.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:50:22.42 +72:53:50.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:50:31.26 +70:07:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:51:07.98 +69:25:24.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:51:35.87 +65:30:23.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:52:46.89 +67:49:23.1 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:44.70 +65:04:14.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:54:50.39 +66:57:16.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:55:33.01 +66:54:52.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:17.91 +70:32:23.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:30.86 +72:51:34.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:57:37.99 +70:38:35.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:58:10.25 +65:24:26.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:15.34 +65:54:52.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:39.30 +71:29:48.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:59:41.46 +67:23:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:00:53.03 +64:54:36.1 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:07.01 +70:03:24.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:01:54.54 +71:44:42.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:11.36 +66:07:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:02:53.69 +65:01:14.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:27.18 +73:34:55.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:33.84 +65:44:44.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:35.97 +68:40:13.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:05:09.09 +66:23:19.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:00.80 +66:58:52.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:10.92 +64:52:32.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:06:50.26 +64:51:24.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:26.76 +73:55:10.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:51.50 +65:22:30.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:07:59.82 +65:47:22.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:11:19.27 +72:08:07.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:11:38.57 +64:54:35.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:11:48.71 +66:41:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:11:49.87 +65:47:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:12:59.98 +68:41:28.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:56.81 +70:34:25.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:15.95 +73:34:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:17:22.73 +71:24:55.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:50.18 +70:16:36.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:19:54.25 +71:34:18.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:32.39 +65:19:26.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:20:36.05 +66:22:28.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:21:43.12 +66:47:48.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:22:24.96 +66:19:03.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:01.23 +71:37:20.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:12.19 +66:12:19.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:25:27.13 +68:03:13.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:27:50.85 +66:14:55.8 -- does not seem to be a hot pixel (will add it to exclusion list)
05:29:55.17 +74:30:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:31:40.78 +70:19:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:33:26.98 +65:17:16.9 -- does not seem to be a hot pixel (will add it to exclusion list)
05:36:09.32 +69:59:53.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:39:11.34 +68:47:03.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:41:41.12 +70:56:51.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:44:28.49 +64:32:52.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:45:20.27 +72:47:19.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:27.89 +68:07:41.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:46:48.60 +66:28:28.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:13.93 +67:04:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:48:20.98 +70:52:48.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:53:03.71 +64:13:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:54:24.56 +67:33:40.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:20.52 +64:07:13.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:55:54.35 +66:08:23.3 -- does not seem to be a hot pixel (will add it to exclusion list)
05:58:17.58 +67:53:45.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:10.95 +71:55:17.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:02:49.55 +66:59:08.9 -- does not seem to be a hot pixel (will add it to exclusion list)
06:03:51.51 +70:17:17.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:05:07.94 +67:40:12.8 -- does not seem to be a hot pixel (will add it to exclusion list)
06:07:07.42 +71:41:37.3 -- does not seem to be a hot pixel (will add it to exclusion list)
06:09:07.02 +72:22:40.1 -- does not seem to be a hot pixel (will add it to exclusion list)
06:23:58.24 +72:38:04.4 -- does not seem to be a hot pixel (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_nohotpixels' -> 'exclusion_list_index_html.txt'
# Count candidates with no identification (that also don't look like hot pix)
03:07:49.50 +72:26:25.5 -- not a known variable star
03:08:09.62 +72:20:39.1 -- not a known variable star
03:08:28.72 +72:22:00.5 -- not a known variable star
03:08:57.58 +72:54:01.9 -- not a known variable star
03:10:42.06 +73:20:48.1 -- not a known variable star
03:10:42.63 +73:30:53.5 -- not a known variable star
03:12:19.68 +71:19:44.4 -- not a known variable star
03:12:38.28 +72:39:11.6 -- not a known variable star
03:13:13.23 +72:32:45.4 -- not a known variable star
03:13:32.43 +71:53:25.2 -- not a known variable star
03:14:45.18 +72:01:17.1 -- not a known variable star
03:14:47.53 +73:15:58.9 -- not a known variable star
03:15:15.25 +70:34:15.1 -- not a known variable star
03:15:24.46 +73:35:27.6 -- not a known variable star
03:17:10.56 +69:54:48.5 -- a known variable star
03:18:08.68 +71:39:25.8 -- not a known variable star
03:22:24.94 +73:47:02.3 -- not a known variable star
03:28:21.89 +70:57:01.0 -- a known variable star
03:43:49.03 +64:45:07.2 -- not a known variable star
03:45:58.45 +68:00:22.8 -- not a known variable star
03:46:01.35 +69:29:05.8 -- not a known variable star
03:53:34.78 +64:50:56.9 -- not a known variable star
03:56:03.26 +69:57:42.2 -- not a known variable star
03:57:23.35 +71:25:00.4 -- not a known variable star
03:57:36.41 +67:28:34.5 -- not a known variable star
03:58:05.38 +65:01:43.4 -- not a known variable star
04:00:27.78 +68:34:39.7 -- not a known variable star
04:00:50.26 +67:35:24.1 -- not a known variable star
04:02:09.32 +70:45:37.7 -- a known variable star
04:02:19.67 +70:42:08.3 -- not a known variable star
04:02:25.59 +66:01:46.0 -- a known variable star
04:05:39.55 +66:19:58.3 -- a known variable star
04:05:44.41 +69:16:50.2 -- not a known variable star
04:05:46.24 +69:03:16.9 -- not a known variable star
04:06:53.12 +65:28:30.0 -- not a known variable star
04:11:33.37 +65:34:23.2 -- not a known variable star
04:12:01.89 +69:32:11.6 -- not a known variable star
04:13:11.73 +67:46:21.7 -- not a known variable star
04:14:47.99 +68:29:38.1 -- not a known variable star
04:15:09.85 +69:56:55.4 -- not a known variable star
04:16:56.09 +69:09:47.9 -- not a known variable star
04:18:00.86 +71:13:59.0 -- a known variable star
04:18:40.67 +74:39:11.6 -- not a known variable star
04:20:01.12 +68:13:26.2 -- not a known variable star
04:20:32.42 +67:29:55.0 -- a known variable star
04:22:14.21 +65:32:26.1 -- not a known variable star
04:24:13.44 +70:35:39.4 -- not a known variable star
04:24:34.32 +67:41:09.7 -- not a known variable star
04:25:21.76 +65:57:39.6 -- not a known variable star
04:25:57.70 +74:11:24.3 -- a known variable star
04:27:04.11 +67:43:40.4 -- not a known variable star
04:29:19.00 +69:15:33.7 -- not a known variable star
04:29:19.56 +69:31:53.2 -- not a known variable star
04:29:42.40 +65:27:15.7 -- not a known variable star
04:29:51.32 +65:59:10.2 -- not a known variable star
04:30:36.89 +74:25:32.2 -- not a known variable star
04:30:48.67 +64:51:50.5 -- not a known variable star
04:32:07.11 +69:05:37.1 -- not a known variable star
04:32:18.16 +66:04:29.9 -- not a known variable star
04:32:28.46 +67:14:27.4 -- not a known variable star
04:32:40.04 +65:00:00.0 -- not a known variable star
04:34:47.55 +66:05:05.8 -- not a known variable star
04:35:53.88 +65:39:42.0 -- a known variable star
04:36:17.78 +72:45:20.9 -- not a known variable star
04:38:34.60 +65:24:55.1 -- not a known variable star
04:39:49.20 +67:53:55.8 -- not a known variable star
04:40:44.63 +71:13:49.0 -- not a known variable star
04:41:09.33 +67:50:57.0 -- not a known variable star
04:41:55.49 +65:26:14.8 -- not a known variable star
04:42:14.52 +69:04:10.6 -- not a known variable star
04:42:25.97 +67:11:09.6 -- not a known variable star
04:42:27.84 +68:36:52.3 -- not a known variable star
04:43:20.69 +72:22:21.8 -- not a known variable star
04:45:55.16 +68:04:57.6 -- not a known variable star
04:49:03.90 +69:07:43.6 -- not a known variable star
04:50:16.69 +72:56:19.2 -- not a known variable star
04:50:22.42 +72:53:50.5 -- not a known variable star
04:50:31.26 +70:07:14.5 -- not a known variable star
04:51:07.98 +69:25:24.9 -- not a known variable star
04:51:35.87 +65:30:23.6 -- not a known variable star
04:52:46.89 +67:49:23.1 -- a known variable star
04:54:44.70 +65:04:14.9 -- a known variable star
04:54:50.39 +66:57:16.6 -- not a known variable star
04:55:33.01 +66:54:52.5 -- not a known variable star
04:56:17.91 +70:32:23.5 -- not a known variable star
04:56:30.86 +72:51:34.2 -- not a known variable star
04:57:37.99 +70:38:35.3 -- not a known variable star
04:58:10.25 +65:24:26.3 -- not a known variable star
04:59:15.34 +65:54:52.3 -- not a known variable star
04:59:39.30 +71:29:48.0 -- not a known variable star
04:59:41.46 +67:23:00.4 -- not a known variable star
05:00:53.03 +64:54:36.1 -- not a known variable star
05:01:07.01 +70:03:24.2 -- not a known variable star
05:01:54.54 +71:44:42.3 -- not a known variable star
05:02:11.36 +66:07:00.4 -- not a known variable star
05:02:53.69 +65:01:14.4 -- not a known variable star
05:03:27.18 +73:34:55.3 -- not a known variable star
05:03:33.84 +65:44:44.7 -- not a known variable star
05:03:35.97 +68:40:13.4 -- not a known variable star
05:05:09.09 +66:23:19.0 -- not a known variable star
05:06:00.80 +66:58:52.0 -- not a known variable star
05:06:10.92 +64:52:32.5 -- not a known variable star
05:06:50.26 +64:51:24.5 -- not a known variable star
05:07:26.76 +73:55:10.8 -- a known variable star
05:07:51.50 +65:22:30.5 -- not a known variable star
05:07:59.82 +65:47:22.8 -- not a known variable star
05:11:19.27 +72:08:07.6 -- not a known variable star
05:11:38.57 +64:54:35.6 -- not a known variable star
05:11:48.71 +66:41:11.0 -- not a known variable star
05:11:49.87 +65:47:00.4 -- not a known variable star
05:12:59.98 +68:41:28.7 -- not a known variable star
05:15:56.81 +70:34:25.3 -- a known variable star
05:17:15.95 +73:34:57.9 -- not a known variable star
05:17:22.73 +71:24:55.0 -- a known variable star
05:19:50.18 +70:16:36.3 -- not a known variable star
05:19:54.25 +71:34:18.4 -- not a known variable star
05:20:32.39 +65:19:26.7 -- not a known variable star
05:20:36.05 +66:22:28.4 -- not a known variable star
05:21:43.12 +66:47:48.5 -- not a known variable star
05:22:24.96 +66:19:03.7 -- not a known variable star
05:24:01.23 +71:37:20.2 -- not a known variable star
05:25:12.19 +66:12:19.7 -- not a known variable star
05:25:27.13 +68:03:13.8 -- not a known variable star
05:27:50.85 +66:14:55.8 -- not a known variable star
05:29:55.17 +74:30:44.9 -- not a known variable star
05:31:40.78 +70:19:44.6 -- a known variable star
05:33:26.98 +65:17:16.9 -- not a known variable star
05:36:09.32 +69:59:53.6 -- not a known variable star
05:39:11.34 +68:47:03.4 -- not a known variable star
05:41:41.12 +70:56:51.2 -- not a known variable star
05:44:28.49 +64:32:52.2 -- not a known variable star
05:45:20.27 +72:47:19.3 -- not a known variable star
05:46:27.89 +68:07:41.2 -- not a known variable star
05:46:48.60 +66:28:28.0 -- a known variable star
05:48:13.93 +67:04:45.2 -- not a known variable star
05:48:20.98 +70:52:48.7 -- a known variable star
05:53:03.71 +64:13:58.4 -- not a known variable star
05:54:24.56 +67:33:40.0 -- not a known variable star
05:55:20.52 +64:07:13.5 -- not a known variable star
05:55:54.35 +66:08:23.3 -- not a known variable star
05:58:17.58 +67:53:45.5 -- a known variable star
06:01:10.95 +71:55:17.3 -- not a known variable star
06:02:49.55 +66:59:08.9 -- not a known variable star
06:03:51.51 +70:17:17.6 -- not a known variable star
06:05:07.94 +67:40:12.8 -- not a known variable star
06:07:07.42 +71:41:37.3 -- not a known variable star
06:09:07.02 +72:22:40.1 -- not a known variable star
06:23:58.24 +72:38:04.4 -- not a known variable star
Found 130 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
148 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 148 (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)2461119.64687559 -observatory 500
22:37:27.27 -07:26:49.5 Mercury (1.1mag)
01:02:41.69 +05:43:08.9 Venus (-3.9mag)
23:00:40.50 -07:29:54.9 Mars (1.2mag)
07:04:39.03 +22:58:08.7 Jupiter (-2.3mag)
00:16:57.51 -00:28:42.0 Saturn (0.9mag)
03:42:48.46 +19:31:26.7 Uranus (5.8mag)
00:07:10.27 -00:38:48.2 Neptune (7.8mag)
20:31:55.72 -22:53:54.8 Pluto (14.5mag)
00:44:48.07 +08:04:27.7 Moon (-8.4mag)
-rw-r--r-- 1 apache apache 361 Mar 19 22:56 planets.txt
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Positions of selected moons from JPL HORIZONS for JD(UT)2461119.64687559:
07:04:30.24 +22:58:25.4 Io (5.6mag)
07:04:40.63 +22:58:01.8 Europa (5.7mag)
07:04:28.69 +22:58:20.4 Ganymede (5.2mag)
07:04:10.01 +22:58:54.2 Callisto (6.4mag)
07:08:40.46 +23:00:15.4 Himalia (15.2mag)
07:04:35.81 +22:58:12.2 Thebe (16.0mag)
07:08:14.29 +23:23:09.3 Elara (17.1mag)
07:01:43.72 +23:52:16.8 Pasiphae (17.2mag)
07:13:27.14 +22:52:26.5 Carme (18.3mag)
00:16:49.39 -00:28:31.4 Titan (8.8mag)
00:16:57.01 -00:28:37.0 Rhea (10.1mag)
00:17:27.89 -00:26:43.4 Iapetus (11.5mag)
00:17:11.68 -00:28:50.3 Hyperion (14.8mag)
00:18:52.09 -00:17:21.7 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 19 22:56 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461119.64687559:
12:42:43.15 +09:45:17.6 JWST
19:30:33.28 +09:16:02.1 Chandra
16:03:53.19 -55:14:26.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 19 22:56 spacecraft.txt
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Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461119.64687559 -observatory 500
18:34:41.00 -27:25:27.3 14.1mag P/2010 H2 (Vales)
04:50:46.27 -71:04:55.8 17.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:28:41.04 +31:17:41.7 17.0mag C/2017 K2 (PANSTARRS)
17:29:29.53 +07:18:09.1 17.6mag C/2021 G2 (ATLAS)
23:01:13.45 +28:25:11.5 16.9mag C/2022 E2 (ATLAS)
03:59:36.96 +25:16:10.7 15.7mag C/2022 N2 (PANSTARRS)
09:01:58.46 +31:24:52.6 16.0mag C/2022 QE78 (ATLAS)
08:30:16.27 -03:17:01.1 17.2mag C/2022 R6 (PANSTARRS)
18:56:28.35 +16:13:07.3 17.5mag C/2023 A3 (Tsuchinshan-ATLAS)
15:46:26.35 -11:51:11.7 17.6mag P/2023 B1 (PANSTARRS)
09:25:14.89 -16:28:42.0 17.4mag C/2023 F3 (ATLAS)
21:20:24.93 +61:40:08.1 17.4mag C/2023 H5 (Lemmon)
19:33:24.72 -03:31:04.4 14.5mag C/2023 R1 (PANSTARRS)
21:35:37.33 +82:46:42.2 17.7mag C/2023 X2 (Lemmon)
06:15:41.63 +63:47:50.8 16.8mag C/2024 A1 (ATLAS)
04:03:38.61 +04:33:40.7 9.0mag C/2024 E1 (Wierzchos)
11:23:20.72 +02:33:42.1 18.0mag C/2024 G2 (ATLAS)
16:32:34.03 +02:01:51.9 17.5mag C/2024 G6 (ATLAS)
20:09:36.13 +08:34:12.7 14.9mag C/2024 J3 (ATLAS)
03:04:03.55 -26:48:11.9 16.5mag C/2024 T5 (ATLAS)
04:57:02.70 +52:52:43.6 17.6mag C/2025 J1 (Borisov)
15:16:03.04 +16:18:50.0 14.4mag C/2025 L1 (ATLAS)
02:47:28.05 -22:28:10.2 17.6mag C/2025 Q3 (ATLAS)
22:32:22.03 +18:57:24.2 12.6mag C/2025 R3 (PANSTARRS)
13:05:23.37 +01:15:19.7 17.7mag C/2025 Y1 (ATLAS)
02:11:52.36 -06:52:22.8 14.3mag C/2026 A1 (MAPS)
22:36:02.23 +30:47:05.8 13.7mag C/2026 B2 (Sun-Gao)
17:50:24.15 -10:51:55.3 13.4mag 10P/Tempel
15:27:10.87 +05:10:49.0 11.7mag 24P/Schaumasse
11:12:21.40 -02:30:50.2 15.6mag 29P/Schwassmann-Wachmann
17:42:46.69 -10:40:40.2 17.3mag 40P/Vaisala
10:45:36.15 -06:39:14.2 16.4mag 43P/Wolf-Harrington
01:07:40.58 +12:46:10.1 17.0mag 47P/Ashbrook-Jackson
06:27:27.07 +42:31:04.6 17.1mag 63P/Wild
22:52:59.98 -14:51:17.6 15.7mag 65P/Gunn
02:56:29.61 +10:57:59.3 15.9mag 76P/West-Kohoutek-Ikemura
00:07:43.36 +02:52:43.4 14.7mag 78P/Gehrels
21:35:47.72 -16:57:45.5 14.5mag 88P/Howell
00:58:36.55 +12:58:20.2 15.3mag 93P/Lovas
04:09:19.69 +30:37:40.9 16.5mag 123P/West-Hartley
08:07:33.99 +50:38:40.7 16.2mag 124P/Mrkos
01:53:06.68 +11:15:09.3 16.4mag 128P/Shoemaker-Holt
01:55:47.28 +10:54:40.2 17.4mag 131P/Mueller
23:16:21.91 +02:45:28.6 13.1mag 141P/Machholz
23:26:26.05 -04:42:10.9 13.1mag 141P-A/Machholz
22:27:44.35 -07:11:14.0 16.2mag 141P-D/Machholz
23:48:02.49 -14:32:22.2 15.5mag 162P/SidingSpring
10:39:57.12 +32:02:13.9 17.5mag 164P/Christensen
05:48:16.23 +24:44:27.5 17.5mag 198P/ODAS
15:34:25.48 -03:29:27.6 16.9mag 210P/Christensen
20:08:33.13 -17:43:38.8 17.1mag 218P/LINEAR
16:58:21.48 -16:44:54.7 16.3mag 235P/LINEAR
04:39:49.79 +31:53:10.4 16.3mag 240P/NEAT
07:29:45.32 -08:29:23.7 17.5mag 242P/Spahr
15:48:36.81 +05:02:26.6 17.7mag 391P/Kowalski
07:27:55.65 +21:05:33.8 17.5mag 450P/LONEOS
04:59:56.18 +46:40:23.1 17.9mag 493P/LONEOS
-rw-r--r-- 1 apache apache 2.8K Mar 19 22:56 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
11:44:44.19 -62:10:45.50 ASASSN-26bq 2026-03-15.03 15.31
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 -0.22
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.41 -74:35:46.80 AT2026ahr 2026-01-20.09 16.98
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:25.13 +04:00:01.40 SN 2026kc 2026-01-18.24 16.4
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
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
-rw-r--r-- 1 apache apache 5.7K Mar 19 22:56 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 19 22:56 tocp_transients_list.txt