This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty
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 02 22.2250 2461093.7250 13.61 04:22:07.89 +70:28:12.0
138.86433 14.43869 galactic Cam Second-epoch detections are separated by 2.4" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:22:07.89 +70:28:12.0 (user input) | T | P | (position from user input) J-Ks=0.648+/-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,2461093.7250,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:22:07.89 +70:28:12.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.56 04:11:43.24 +72:22:00.2
136.85792 15.16026 galactic Cam Second-epoch detections are separated by 6.4" and 4.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:11:43.24 +72:22:00.2 (user input) | T | P | (position from user input) J-Ks=0.617+/-0.039 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:11:43.24 +72:22:00.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.48 03:30:26.93 +72:12:32.3
134.50026 13.00950 galactic Cas Second-epoch detections are separated by 6.1" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:30:26.93 +72:12:32.3 (user input) | T | P | (position from user input) J-Ks=0.492+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2250* 03 30 26.93 +72 12 32.3 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:30:26.93 +72:12:32.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.37 04:24:10.41 +70:35:43.5
138.88872 14.64873 galactic Cam Second-epoch detections are separated by 2.9" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:24:10.41 +70:35:43.5 (user input) | T | P | (position from user input) J-Ks=0.445+/-0.040 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:10.41 +70:35:43.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:06:36.98 +68:36:18.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 492786341181004672,2461093.7250,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 492786341181004672 20260222.2250 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:34:12.73 +68:05:38.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2250* 03 33 14.42 +73 11 24.6 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:33:14.42 +73:11:24.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.24,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 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-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:40:05.95 +66:51:06.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 543689846896570368,2461093.7250,13.19,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 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 543689846896570368 20260222.2250 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-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:44:34.02 +72:43:45.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 12.96 04:07:04.74 +71:00:54.0
137.56495 13.93897 galactic Cam Second-epoch detections are separated by 2.1" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:07:04.74 +71:00:54.0 (user input) | T | P | (position from user input) J-Ks=0.315+/-0.032 (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,2461093.7250,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:07:04.74 +71:00:54.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 12.93 04:21:55.21 +72:14:51.9
137.50390 15.63643 galactic Cam Second-epoch detections are separated by 1.3" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:21:55.21 +72:14:51.9 (user input) | T | P | (position from user input) J-Ks=0.413+/-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,2461093.7250,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:21:55.21 +72:14:51.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.02 03:37:07.46 +75:03:28.5
133.13220 15.57442 galactic Cas Second-epoch detections are separated by 4.2" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:37:07.46 +75:03:28.5 (user input) | T | P | (position from user input) J-Ks=0.425+/-0.037 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2250* 03 37 07.46 +75 03 28.5 13.0 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,2461093.7250,13.02,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.02CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:07.46 +75:03:28.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 12.71 03:36:06.27 +74:10:08.1
133.63727 14.82787 galactic Cas Second-epoch detections are separated by 3.6" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:36:06.27 +74:10:08.1 (user input) | T | P | (position from user input) J-Ks=0.314+/-0.038 (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!
TCP 2026 02 22.2250* 03 36 06.27 +74 10 08.1 12.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:36:06.27 +74:10:08.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 12.71 03:47:56.15 +67:53:18.8
138.38882 10.48483 galactic Cam Second-epoch detections are separated by 1.7" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 493284557383018368 | 03:47:56.15 +67:53:18.8 (user input) | 2021A&A...648A..44M | | (position from user input) (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification) J-Ks=0.488+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 493284557383018368,2461093.7250,12.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 493284557383018368 20260222.2250 12.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:56.15 +67:53:18.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 10.85 03:44:24.30 +67:06:02.1
138.62039 9.65837 galactic Cam Second-epoch detections are separated by 4.7" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 493224805802407552 | 03:44:22.23 +67:06:22.7 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.494+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 493224805802407552,2461093.7250,10.85,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493224805802407552 20260222.2250 10.85CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:44:24.30 +67:06:02.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 11.74 04:17:40.79 +73:11:40.6
136.56178 16.05381 galactic Cam Second-epoch detections are separated by 3.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 501531135112056448 | 04:17:49.19 +73:11:40.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.698+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 501531135112056448,2461093.7250,11.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 501531135112056448 20260222.2250 11.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:17:40.79 +73:11:40.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 12.17 03:58:02.50 +65:53:36.7
140.46289 9.59568 galactic Cam Second-epoch detections are separated by 1.9" and 5.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 489831747279814400 | 03:58:06.32 +65:53:34.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.555+/-0.034 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 489831747279814400,2461093.7250,12.17,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 489831747279814400 20260222.2250 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-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:58:02.50 +65:53:36.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 12.29 03:55:21.70 +67:27:31.8
139.21960 10.60676 galactic Cam Second-epoch detections are separated by 4.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | CzeV3511 | 03:55:25.97 +67:27:45.3 (Gaia DR3) | DSCT (local) | 0.117351000000 (local) | Gaia3var=NOT_AVAILABLE J-Ks=0.358+/-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
CzeV3511,2461093.7250,12.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CzeV3511 20260222.2250 12.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:55:21.70 +67:27:31.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 12.45 03:44:23.74 +69:26:47.6
137.13934 11.49799 galactic Cam Second-epoch detections are separated by 0.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 494493951459077632 | 03:44:25.56 +69:27:07.4 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.554+/-0.034 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 494493951459077632,2461093.7250,12.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 494493951459077632 20260222.2250 12.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:44:23.74 +69:26:47.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 12.79 03:45:20.81 +72:59:30.3
134.92002 14.30789 galactic Cam Second-epoch detections are separated by 2.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 543701666645486592 | 03:45:28.68 +72:59:25.2 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: M0 1985ApJS...59..197B LTT 11224
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 543701666645486592,2461093.7250,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543701666645486592 20260222.2250 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:20.81 +72:59:30.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.29 03:37:21.19 +68:07:11.7
137.44998 10.05839 galactic Cam Second-epoch detections are separated by 3.9" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:37:21.19 +68:07:11.7 (user input) | T | P | (position from user input) J-Ks=0.480+/-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,2461093.7250,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:21.19 +68:07:11.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2250* 03 37 30.19 +73 05 58.2 13.3 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:30.19 +73:05:58.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.16 03:47:19.19 +68:48:45.6
137.75117 11.16671 galactic Cam Second-epoch detections are separated by 0.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:47:19.19 +68:48:45.6 (user input) | T | P | (position from user input) J-Ks=0.746+/-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,2461093.7250,13.16,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.16CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:19.19 +68:48:45.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.29 03:45:42.61 +66:24:56.9
139.15314 9.20088 galactic Cam Second-epoch detections are separated by 5.1" and 5.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:45:42.61 +66:24:56.9 (user input) | T | P | (position from user input) J-Ks=0.504+/-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,2461093.7250,13.29,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.29CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:42.61 +66:24:56.9 ;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-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.22 04:13:48.34 +71:34:09.3
137.56088 14.71230 galactic Cam Second-epoch detections are separated by 2.6" and 5.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:13:48.34 +71:34:09.3 (user input) | T | P | (position from user input) J-Ks=0.694+/-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,2461093.7250,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.22CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:13:48.34 +71:34:09.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:35:17.32 +68:00:58.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:45:33.34 +73:23:58.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:12:16.14 +73:13:02.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.38 03:41:55.86 +68:36:21.9
137.49170 10.70083 galactic Cam Second-epoch detections are separated by 0.0" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:41:55.86 +68:36:21.9 (user input) | T | P | (position from user input) J-Ks=0.442+/-0.035 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.38,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.38CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:55.86 +68:36:21.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.44 03:41:46.99 +74:26:29.0
133.77721 15.27892 galactic Cam Second-epoch detections are separated by 3.3" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:41:46.99 +74:26:29.0 (user input) | T | P | (position from user input) J-Ks=0.459+/-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,2461093.7250,13.44,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.44CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:46.99 +74:26:29.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.45 03:33:51.02 +73:27:45.7
133.94660 14.16929 galactic Cas Second-epoch detections are separated by 2.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:33:51.02 +73:27:45.7 (user input) | T | P | (position from user input) J-Ks=0.533+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2250* 03 33 51.02 +73 27 45.7 13.4 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:33:51.02 +73:27:45.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.40 03:33:48.89 +67:50:05.6
137.35048 9.63220 galactic Cam Second-epoch detections are separated by 5.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:33:48.89 +67:50:05.6 (user input) | T | P | (position from user input) J-Ks=0.585+/-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,2461093.7250,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:33:48.89 +67:50:05.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.39 03:46:42.92 +68:52:25.6
137.66877 11.17991 galactic Cam Second-epoch detections are separated by 1.6" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:46:42.92 +68:52:25.6 (user input) | T | P | (position from user input) J-Ks=0.522+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.39,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.39CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:42.92 +68:52:25.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.64,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.64CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:08.08 +73:08:36.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.46 03:53:53.89 +71:11:44.6
136.62745 13.35497 galactic Cam Second-epoch detections are separated by 2.4" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:53:53.89 +71:11:44.6 (user input) | T | P | (position from user input) J-Ks=0.505+/-0.057 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:53.89 +71:11:44.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.45 04:05:44.83 +75:02:47.8
134.59083 16.77453 galactic Cam Second-epoch detections are separated by 5.1" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:05:44.83 +75:02:47.8 (user input) | T | P | (position from user input) J-Ks=0.325+/-0.043 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:05:44.83 +75:02:47.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2250* 03 32 08.02 +69 08 21.9 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:32:08.02 +69:08:21.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.65 03:52:15.61 +70:37:25.1
136.90525 12.83344 galactic Cam Second-epoch detections are separated by 1.5" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:52:15.61 +70:37:25.1 (user input) | T | P | (position from user input) J-Ks=0.755+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:15.61 +70:37:25.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.72 03:41:17.35 +68:48:39.3
137.31711 10.82705 galactic Cam Second-epoch detections are separated by 0.8" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:41:17.35 +68:48:39.3 (user input) | T | P | (position from user input) J-Ks=0.597+/-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,2461093.7250,13.72,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.72CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:17.35 +68:48:39.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.60 03:53:27.59 +67:28:22.1
139.06927 10.49925 galactic Cam Second-epoch detections are separated by 3.6" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:53:27.59 +67:28:22.1 (user input) | T | P | (position from user input) J-Ks=0.575+/-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,2461093.7250,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:27.59 +67:28:22.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.52 03:29:14.31 +73:23:41.4
133.71420 13.92049 galactic Cas Second-epoch detections are separated by 4.3" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:29:14.31 +73:23:41.4 (user input) | T | P | (position from user input) J-Ks=0.405+/-0.037 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2250* 03 29 14.31 +73 23 41.4 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:29:14.31 +73:23:41.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 495103802454134528,2461093.7250,13.62,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 495103802454134528 20260222.2250 13.62CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:01:43.33 +71:19:26.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2250* 03 34 02.50 +70 34 00.4 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.46,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.46CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:34:02.50 +70:34:00.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2250* 03 37 42.95 +74 38 57.9 13.5 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:42.95 +74:38:57.9 ;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-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:06.60 +65:09:29.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.49,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.49CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:17.36 +72:57:36.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.57 04:24:56.33 +71:25:51.5
138.29357 15.25817 galactic Cam Second-epoch detections are separated by 4.6" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 500353175905353088 | 04:24:54.02 +71:26:25.0 (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 500353175905353088,2461093.7250,13.57,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 500353175905353088 20260222.2250 13.57CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:56.33 +71:25:51.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.71 03:27:27.77 +69:26:12.1
135.92975 10.60372 galactic Cas Second-epoch detections are separated by 3.5" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:27:27.77 +69:26:12.1 (user input) | T | P | (position from user input) J-Ks=0.701+/-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!
TCP 2026 02 22.2250* 03 27 27.77 +69 26 12.1 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:27:27.77 +69:26:12.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.69 03:40:12.87 +71:31:30.6
135.54475 12.91691 galactic Cam Second-epoch detections are separated by 2.4" and 4.9 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:40:12.87 +71:31:30.6 (user input) | T | P | (position from user input) J-Ks=0.359+/-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,2461093.7250,13.69,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.69CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:40:12.87 +71:31:30.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 543456230741626112,2461093.7250,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 543456230741626112 20260222.2250 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:57:21.93 +72:37:57.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.58,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.58CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:29.69 +69:01:42.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.74 03:35:58.63 +69:09:52.1
136.71333 10.82126 galactic Cas Second-epoch detections are separated by 1.0" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:35:58.63 +69:09:52.1 (user input) | T | P | (position from user input) J-Ks=0.453+/-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!
TCP 2026 02 22.2250* 03 35 58.63 +69 09 52.1 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.74,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.74CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:35:58.63 +69:09:52.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.60 03:47:15.21 +66:33:58.4
139.17996 9.41445 galactic Cam Second-epoch detections are separated by 0.9" and 4.8 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:47:15.21 +66:33:58.4 (user input) | T | P | (position from user input) J-Ks=0.767+/-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,2461093.7250,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:47:15.21 +66:33:58.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2250* 03 32 05.72 +73 26 20.0 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:32:05.72 +73:26:20.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.75 03:30:12.28 +70:22:44.4
135.57401 11.51007 galactic Cas Second-epoch detections are separated by 7.5" and 4.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:30:12.28 +70:22:44.4 (user input) | T | P | (position from user input) J-Ks=0.559+/-0.033 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2250* 03 30 12.28 +70 22 44.4 13.8 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:30:12.28 +70:22:44.4 ;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-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.79 03:40:42.61 +72:13:18.2
135.13617 13.49001 galactic Cam Second-epoch detections are separated by 2.7" and 4.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:40:42.61 +72:13:18.2 (user input) | T | P | (position from user input) J-Ks=0.587+/-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,2461093.7250,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:40:42.61 +72:13:18.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 494527864519891712,2461093.7250,13.68,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 494527864519891712 20260222.2250 13.68CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:48:18.46 +69:46:49.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.75 03:43:51.78 +74:14:46.2
134.01740 15.21491 galactic Cam Second-epoch detections are separated by 1.5" and 5.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:43:51.78 +74:14:46.2 (user input) | T | P | (position from user input) J-Ks=0.407+/-0.053 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:43:51.78 +74:14:46.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.75,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.75CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:17:23.69 +72:57:04.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.70 03:38:08.92 +71:58:09.3
135.13494 13.16986 galactic Cam Second-epoch detections are separated by 4.6" and 4.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:38:08.92 +71:58:09.3 (user input) | T | P | (position from user input) J-Ks=0.552+/-0.076 (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,2461093.7250,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:38:08.92 +71:58:09.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 494746255016239616,2461093.7250,13.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 494746255016239616 20260222.2250 13.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:03.55 +70:03:53.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.66 03:49:42.41 +67:23:18.1
138.84300 10.20387 galactic Cam Second-epoch detections are separated by 2.0" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:49:42.41 +67:23:18.1 (user input) | T | P | (position from user input) J-Ks=0.609+/-0.030 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:42.41 +67:23:18.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
WISE J034040.7+691739,2461093.7250,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WISE J034040.7+691739 20260222.2250 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:40:40.64 +69:17:39.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.70,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.70CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:35.04 +67:41:58.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2250* 03 32 51.59 +74 13 55.9 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 544815471923961344,2461093.7250,13.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 544815471923961344 20260222.2250 13.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:32:51.59 +74:13:55.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2250* 03 36 58.79 +69 03 32.9 13.7 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
CzeV772,2461093.7250,13.66,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CzeV772 20260222.2250 13.66CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:36:58.79 +69:03:32.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.56 03:41:25.58 +68:24:24.3
137.57872 10.51494 galactic Cam Second-epoch detections are separated by 4.2" and 5.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:41:25.58 +68:24:24.3 (user input) | T | P | (position from user input) J-Ks=0.416+/-0.038 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.56,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.56CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:25.58 +68:24:24.3 ;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-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.82 03:38:29.72 +66:47:58.3
138.34152 9.06718 galactic Cam Second-epoch detections are separated by 4.3" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:38:29.72 +66:47:58.3 (user input) | T | P | (position from user input) J-Ks=0.520+/-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,2461093.7250,13.82,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.82CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:38:29.72 +66:47:58.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 02 22.2250* 03 34 41.16 +72 06 53.7 13.6 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461093.7250,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:34:41.16 +72:06:53.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 02 22.2250 2461093.7250 13.81 03:52:43.90 +73:25:45.1
135.05089 14.98587 galactic Cam Second-epoch detections are separated by 1.0" and 5.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:52:43.90 +73:25:45.1 (user input) | T | P | (position from user input) J-Ks=0.482+/-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,2461093.7250,13.81,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260222.2250 13.81CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:52:43.90 +73:25:45.1 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 494324832826178688,2461093.7250,13.61,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-1 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 494324832826178688 20260222.2250 13.61CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:38:24.67 +68:37:37.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20_00sec_-14_90C_LIGHT_0212_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20_00sec_-14_90C_LIGHT_0211_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
First image: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Last image: 2461093.72527366 22.02.2026 05:24:13.644 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 10
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: 11 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): 16287
Objects passed selection criteria: 16279
Measurements per detected object (mean, median, min, max): 3.8 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.8 4.0 2 4
Average stars detected per image: 15789.8
Average stars matched: 15395 (97.5 %)
Memory usage VmPeak: 120640 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 02:38:15 CST 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
First image: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Last image: 2461093.72527366 22.02.2026 05:24:13.644 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 331
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: 70 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): 114477
Objects passed selection criteria: 114174
Measurements per detected object (mean, median, min, max): 3.7 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.7 4.0 2 4
Average stars detected per image: 109973
Average stars matched: 105862 (96.2611 %)
Memory usage VmPeak: 1897456 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Wed Feb 11 15:05:05 CST 2026
VaST build number 1.0rc88-300-g65540497
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-02-11)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Feb 22 02:46:43 CST 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ1b1x1/TTUQ1_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
SExtractor catalog cache: saved Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat to cache
SExtractor catalog cache: saved Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.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: 2461093.72475690
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Re-using ../tocp_transients_list.txt
'../tocp_transients_list.txt' -> 'tocp_transients_list.txt'
Plate-solving the images
wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits exists and is non-empty
Saving wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits to local_wcs_cache/
'wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> 'local_wcs_cache/wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits'
wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits exists and is non-empty
Saving wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits to local_wcs_cache/
'wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> 'local_wcs_cache/wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits'
wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits'
wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.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 04:47:37.734 +70:00:56.45
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 04:47:56.079 +69:59:29.08
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:47:37.734 +70:00:56.45
Second-epoch second image center 04:47:56.079 +69:59:29.08
Angular distance between the image centers 0.03567 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits &> /tmp/tmp.fFLmzVx9U9
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits &> /tmp/tmp.diFaMRuDy8
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits &> /tmp/tmp.e4QUMsofTb
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits &> /tmp/tmp.GyKMBzCTHf
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Found non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
The reference image (wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits) and catalog (wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat) found
'wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 58 out of 16183 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 22.881698
a=0.000000 b=1.000000 c=22.881698
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.26
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.26
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 9 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
2.1 pix Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
2.2 pix fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
2.2 pix fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
Limiting magnitude estimates:
15.3 mag. Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
15.2 mag. Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
15.2 mag. fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
15.2 mag. fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
All-image limiting magnitude estimate: 15.2 (SNR ) 12.2 (80% of stars) with default.sex.telephoto_lens_onlybrightstars_v1
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.fFLmzVx9U9 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> 'wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS-calibrated image found: wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Checking if the catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS catalog name: wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1300, passed=16183
Got 16183 stars (including 14865 good ones) from the SExtractor catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
util/solve_plate_with_UCAC5 got 16183 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.3'
Seting catalog search parameters based on the expected field of view 931.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012935 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010348 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 292 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.79"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.09"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 360 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.02"
Estimated accuracy of the plate solution: 5.56"
Excluding outliers - 323 stars left (next iteration limit 245)
The image catalog is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits -region wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.diFaMRuDy8 (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> 'wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Checking if the catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS catalog name: wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1282, passed=16167
Got 16167 stars (including 14867 good ones) from the SExtractor catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat
util/solve_plate_with_UCAC5 got 16167 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits -region wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.e4QUMsofTb (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
Checking if the catalog wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
WCS catalog name: wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1264, passed=15604
Got 15604 stars (including 14332 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits.cat
util/solve_plate_with_UCAC5 got 15604 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.4'
Seting catalog search parameters based on the expected field of view 931.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012936 (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 0.010349 (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 281 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: 6.52"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.25"
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 342 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.17"
Estimated accuracy of the plate solution: 5.84"
Excluding outliers - 309 stars left (next iteration limit 242)
The image catalog is written to wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits -region wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.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.GyKMBzCTHf (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
Checking if the catalog wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
WCS catalog name: wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1272, passed=15547
Got 15547 stars (including 14262 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits.cat
util/solve_plate_with_UCAC5 got 15547 stars from the SExtractor catalog
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/util/fov_of_wcs_calibrated_image.sh: line 144: echo: write error: Broken pipe
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 971 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: 0.47"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.44"
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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.44"
Estimated accuracy of the plate solution: 0.43"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits -region wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits'
Saving fully-calibrated image wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits'
Preparing the HTML report for the field Cam-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
make_report_in_HTML.sh Phase 1 (network queries): 0s
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
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21065_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 21065_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (9.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21066_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 21066_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (268.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21069_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 21069_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (172.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21075_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 21075_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (98.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21077_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 21077_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (490.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21078_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 21078_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (456.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21079_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 21079_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (215.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21086_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 21086_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (451.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21090_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 21090_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (333.1") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cam-06-Q1b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 3.5 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
SExtractor catalog cache: saved Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat to cache
SExtractor catalog cache: saved Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Creating symlink local_wcs_cache/wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits exists and is non-empty
wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits exists and is non-empty
wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits exists and is non-empty
wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.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 04:47:37.734 +70:00:56.45
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 04:47:56.079 +69:59:29.08
Angular distance between the image centers 0.02 deg.
###################################
###################################
# Check the image center offset between the first and the second second-epoch image (shift should be applied between the second-epoch images)
Second-epoch first image center 04:47:37.734 +70:00:56.45
Second-epoch second image center 04:47:56.079 +69:59:29.08
Angular distance between the image centers 0.03567 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits &> /tmp/tmp.Gt6i08I1iK
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits &> /tmp/tmp.yuIlbAOSMo
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits &> /tmp/tmp.QMua5R73SA
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits &> /tmp/tmp.NebXztHIik
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Found non-empty wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
The reference image (wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits) and catalog (wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat) found
'wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 85 out of 113524 detected stars.
util/calibrate_magnitude_scale 0.000000 1.000000 21.485425
a=0.000000 b=1.000000 c=21.485425
From vast_summary.log: estimated ref. image limiting mag.: -7.31
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.18
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.18
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 287 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
1.9 pix Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
2.0 pix fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
2.0 pix fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
Limiting magnitude estimates:
14.2 mag. Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
14.2 mag. Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
14.1 mag. fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
14.1 mag. fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
All-image limiting magnitude estimate: 14.1 (SNR ) 13.4 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 14.5 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.Gt6i08I1iK (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> 'wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS-calibrated image found: wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Checking if the catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS catalog name: wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=9713, passed=113493
Got 113493 stars (including 103609 good ones) from the SExtractor catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
util/solve_plate_with_UCAC5 got 113493 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.3'
Seting catalog search parameters based on the expected field of view 931.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012935 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010348 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 303 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 368 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.45"
Estimated accuracy of the plate solution: 5.59"
Excluding outliers - 329 stars left (next iteration limit 266)
The image catalog is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits -region wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.yuIlbAOSMo (6) ############
Parsing command line arguments...
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> 'wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Checking if the catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS catalog name: wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=9545, passed=112768
Got 112768 stars (including 103038 good ones) from the SExtractor catalog wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat
util/solve_plate_with_UCAC5 got 112768 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits -region wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q1b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.QMua5R73SA (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
Checking if the catalog wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
WCS catalog name: wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=9782, passed=108267
Got 108267 stars (including 98310 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits.cat
util/solve_plate_with_UCAC5 got 108267 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.4'
Seting catalog search parameters based on the expected field of view 931.4 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012936 (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 0.010349 (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 299 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: 6.51"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.07"
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 363 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.06"
Estimated accuracy of the plate solution: 5.79"
Excluding outliers - 334 stars left (next iteration limit 262)
The image catalog is written to wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits -region wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.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.NebXztHIik (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
Checking if the catalog wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits.cat corresponding to the image wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
WCS catalog name: wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=44, blended=9741, passed=108123
Got 108123 stars (including 98206 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits.cat
util/solve_plate_with_UCAC5 got 108123 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.9'
Seting catalog search parameters based on the expected field of view 941.9 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013082 (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 0.010466 (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 971 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: 0.45"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.45"
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 971 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.45"
Estimated accuracy of the plate solution: 0.44"
Excluding outliers - 970 stars left (next iteration limit 1067)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits -region wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-23-28_20.00sec_-14.90C_LIGHT_0211.fits
Saving fully-calibrated image wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-02-21_CI_Cam-06-Q1b1x1_232619_TTUQ1b1x1_1266_3fvyusty/wcs_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212.fits
Preparing the HTML report for the field Cam-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out133053.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133101.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133942.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out134162.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out133035.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133062.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133069.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133121.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133124.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133128.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133129.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133140.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133148.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133150.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133152.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133157.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133160.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133236.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133288.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133345.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133365.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133376.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133426.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133533.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133550.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133564.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133573.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133608.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133612.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133639.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133643.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133683.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133684.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133690.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133699.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133708.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133724.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133729.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133762.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133783.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133806.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133810.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133854.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133874.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133894.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133903.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133922.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133950.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133952.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133961.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133966.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134015.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134028.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134038.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134040.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134056.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134061.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134070.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134078.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134097.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134105.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134133.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134143.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134167.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134168.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134169.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134171.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134204.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134215.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134224.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134228.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134232.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 131s
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: 49s
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Considering the candidate 133025_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133025_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (636.8") between the two second-epoch detections
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Considering the candidate 133035_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133035_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133036_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133036_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (197.0") between the two second-epoch detections
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Considering the candidate 133039_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133039_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (200.3") between the two second-epoch detections
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Considering the candidate 133041_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133041_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (38.8") between the two second-epoch detections
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Considering the candidate 133049_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133049_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (293.1") between the two second-epoch detections
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Considering the candidate 133051_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133051_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (31.3") between the two second-epoch detections
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Considering the candidate 133053_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133053_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 03:44:15.82 +70:02:53.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.54, MAG_FAINT_SEARCH_LIMIT=14.52)GAIADR2_OUTPUT=# 2.093 494737424563690880 056.06616296843 +70.04868646495 14.5156 13.5159 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.093#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133055_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133055_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (402.8") between the two second-epoch detections
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Considering the candidate 133056_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133056_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (66.7") between the two second-epoch detections
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Considering the candidate 133057_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133057_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (137.2") between the two second-epoch detections
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Considering the candidate 133058_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133058_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (256.5") between the two second-epoch detections
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Considering the candidate 133060_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133060_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (459.3") between the two second-epoch detections
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Considering the candidate 133061_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133061_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (480.5") between the two second-epoch detections
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Considering the candidate 133062_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133062_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133064_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133064_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (194.1") between the two second-epoch detections
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Considering the candidate 133065_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133065_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (261.7") between the two second-epoch detections
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Considering the candidate 133068_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133068_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (481.6") between the two second-epoch detections
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Considering the candidate 133069_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133069_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133070_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133070_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (295.5") between the two second-epoch detections
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Considering the candidate 133071_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133071_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (779.0") between the two second-epoch detections
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Considering the candidate 133072_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133072_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (127.3") between the two second-epoch detections
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Considering the candidate 133074_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133074_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (239.4") between the two second-epoch detections
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Considering the candidate 133082_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133082_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (166.4") between the two second-epoch detections
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Considering the candidate 133086_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133086_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (16.9") between the two second-epoch detections
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Considering the candidate 133090_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133090_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (344.4") between the two second-epoch detections
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Considering the candidate 133094_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133094_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (697.6") between the two second-epoch detections
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Considering the candidate 133096_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133096_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (70.9") between the two second-epoch detections
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Considering the candidate 133100_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133100_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (522.6") between the two second-epoch detections
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Considering the candidate 133101_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133101_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 04:05:33.51 +68:09:45.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.39, MAG_FAINT_SEARCH_LIMIT=14.37)GAIADR2_OUTPUT=# 1.481 490722454775549312 061.39040952992 +68.16229329100 14.2074 13.2492 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.481#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133102_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133102_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (536.0") between the two second-epoch detections
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Considering the candidate 133105_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133105_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133113_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133113_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (132.1") between the two second-epoch detections
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Considering the candidate 133114_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133114_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (165.0") between the two second-epoch detections
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Considering the candidate 133115_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133115_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (648.0") between the two second-epoch detections
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Considering the candidate 133121_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133121_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133123_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133123_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (702.3") between the two second-epoch detections
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Considering the candidate 133124_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133124_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133127_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133127_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (295.5") between the two second-epoch detections
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Considering the candidate 133128_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133128_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133129_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133129_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133130_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133130_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (188.5") between the two second-epoch detections
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Considering the candidate 133133_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133133_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (150.3") between the two second-epoch detections
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Considering the candidate 133140_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133140_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133145_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133145_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (231.5") between the two second-epoch detections
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Considering the candidate 133148_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133148_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133150_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133150_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133151_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133151_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (141.8") between the two second-epoch detections
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Considering the candidate 133152_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133152_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133154_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133154_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (413.7") between the two second-epoch detections
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Considering the candidate 133157_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133157_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133160_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133160_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133163_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133163_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (408.0") between the two second-epoch detections
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Considering the candidate 133167_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133167_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 03:45:47.21 +73:18:30.6 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133169_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133169_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (283.0") between the two second-epoch detections
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Considering the candidate 133170_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133170_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (35.7") between the two second-epoch detections
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Considering the candidate 133173_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133173_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (48.8") between the two second-epoch detections
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Considering the candidate 133176_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133176_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (391.2") between the two second-epoch detections
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Considering the candidate 133179_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133179_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (437.3") between the two second-epoch detections
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Considering the candidate 133181_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133181_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (198.8") between the two second-epoch detections
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Considering the candidate 133184_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133184_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (233.1") between the two second-epoch detections
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Considering the candidate 133185_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133185_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (517.6") between the two second-epoch detections
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Considering the candidate 133186_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133186_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (43.6") between the two second-epoch detections
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Considering the candidate 133188_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133188_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (118.8") between the two second-epoch detections
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Considering the candidate 133190_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133190_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (647.4") between the two second-epoch detections
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Considering the candidate 133191_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133191_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (122.6") between the two second-epoch detections
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Considering the candidate 133236_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133236_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133288_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133288_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133324_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133324_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (121.8") between the two second-epoch detections
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Considering the candidate 133345_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133345_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133365_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133365_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133376_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133376_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133385_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133385_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (53.3") between the two second-epoch detections
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Considering the candidate 133389_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133389_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 03:38:07.08 +71:44:57.4 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133426_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133426_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133447_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133447_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (192.5") between the two second-epoch detections
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Considering the candidate 133452_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133452_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (321.6") between the two second-epoch detections
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Considering the candidate 133472_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133472_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (52.5") between the two second-epoch detections
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Considering the candidate 133481_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133481_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (121.3") between the two second-epoch detections
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Considering the candidate 133483_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133483_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (226.3") between the two second-epoch detections
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Considering the candidate 133500_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133500_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (427.5") between the two second-epoch detections
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Considering the candidate 133533_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133533_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133535_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133535_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (187.3") between the two second-epoch detections
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Considering the candidate 133550_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133550_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133564_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133564_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133565_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133565_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (270.4") between the two second-epoch detections
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Considering the candidate 133568_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133568_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (71.9") between the two second-epoch detections
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Considering the candidate 133573_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133573_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133578_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133578_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (46.0") between the two second-epoch detections
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Considering the candidate 133579_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133579_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (34.6") between the two second-epoch detections
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Considering the candidate 133582_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133582_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (426.9") between the two second-epoch detections
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Considering the candidate 133583_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133583_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (42.1") between the two second-epoch detections
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Considering the candidate 133590_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133590_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (533.7") between the two second-epoch detections
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Considering the candidate 133598_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133598_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (125.2") between the two second-epoch detections
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Considering the candidate 133599_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133599_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (15.3") between the two second-epoch detections
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Considering the candidate 133605_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133605_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (40.4") between the two second-epoch detections
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Considering the candidate 133606_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133606_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (167.4") between the two second-epoch detections
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Considering the candidate 133608_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133608_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133612_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133612_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133614_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133614_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (640.1") between the two second-epoch detections
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Considering the candidate 133625_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133625_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 03:54:25.27 +65:04:18.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133630_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133630_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (122.3") between the two second-epoch detections
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Considering the candidate 133634_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133634_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (407.4") between the two second-epoch detections
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Considering the candidate 133637_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133637_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 03:43:14.92 +71:23:51.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133639_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133639_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133643_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133643_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133645_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133645_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (115.5") between the two second-epoch detections
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Considering the candidate 133649_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133649_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (9.9") between the two second-epoch detections
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Considering the candidate 133654_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133654_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (17.8") between the two second-epoch detections
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Considering the candidate 133658_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133658_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (49.5") between the two second-epoch detections
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Considering the candidate 133661_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133661_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (96.7") between the two second-epoch detections
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Considering the candidate 133669_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133669_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (55.4") between the two second-epoch detections
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Considering the candidate 133670_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133670_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 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 133671_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133671_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (111.3") between the two second-epoch detections
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Considering the candidate 133673_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133673_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (86.2") between the two second-epoch detections
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Considering the candidate 133674_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133674_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (432.8") between the two second-epoch detections
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Considering the candidate 133675_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133675_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 03:43:33.56 +70:59:15.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133683_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133683_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133684_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133684_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133690_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133690_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133696_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133696_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (406.9") between the two second-epoch detections
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Considering the candidate 133698_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133698_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (120.6") between the two second-epoch detections
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Considering the candidate 133699_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133699_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133700_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133700_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (91.0") between the two second-epoch detections
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Considering the candidate 133704_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133704_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (578.5") between the two second-epoch detections
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Considering the candidate 133706_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133706_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (790.9") between the two second-epoch detections
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Considering the candidate 133708_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133708_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133711_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133711_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (111.8") between the two second-epoch detections
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Considering the candidate 133716_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133716_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (127.1") between the two second-epoch detections
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Considering the candidate 133717_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133717_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (273.8") between the two second-epoch detections
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Considering the candidate 133718_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133718_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (299.0") between the two second-epoch detections
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Considering the candidate 133724_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133724_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133728_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133728_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 03:39:31.42 +69:18:52.7 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133729_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133729_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133730_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133730_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 03:33:29.06 +72:29:19.3 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133735_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133735_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (455.8") between the two second-epoch detections
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Considering the candidate 133739_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133739_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (57.7") between the two second-epoch detections
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Considering the candidate 133740_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133740_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (52.3") between the two second-epoch detections
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Considering the candidate 133744_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133744_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (75.3") between the two second-epoch detections
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Considering the candidate 133745_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133745_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (22.5") between the two second-epoch detections
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Considering the candidate 133751_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133751_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133760_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133760_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (22.1") between the two second-epoch detections
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Considering the candidate 133762_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133762_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133770_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133770_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (756.6") between the two second-epoch detections
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Considering the candidate 133771_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133771_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (147.2") between the two second-epoch detections
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Considering the candidate 133772_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133772_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (607.7") between the two second-epoch detections
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Considering the candidate 133774_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133774_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (41.0") between the two second-epoch detections
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Considering the candidate 133776_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133776_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (63.3") between the two second-epoch detections
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Considering the candidate 133783_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133783_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133788_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133788_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (10.6") between the two second-epoch detections
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Considering the candidate 133791_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133791_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (740.2") between the two second-epoch detections
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Considering the candidate 133792_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133792_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 03:54:38.95 +68:08:21.5 in the exclusion list exclusion_list.txt ****
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Considering the candidate 133794_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133794_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
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Considering the candidate 133802_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133802_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (22.8") between the two second-epoch detections
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Considering the candidate 133806_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133806_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133810_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133810_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133827_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133827_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (34.9") between the two second-epoch detections
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Considering the candidate 133828_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133828_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (438.9") between the two second-epoch detections
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Considering the candidate 133829_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133829_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (639.7") between the two second-epoch detections
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Considering the candidate 133836_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133836_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (727.5") between the two second-epoch detections
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Considering the candidate 133837_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133837_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (104.2") between the two second-epoch detections
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Considering the candidate 133843_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133843_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (116.9") between the two second-epoch detections
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Considering the candidate 133844_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133844_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (30.7") between the two second-epoch detections
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Considering the candidate 133848_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133848_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (683.0") between the two second-epoch detections
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Considering the candidate 133850_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133850_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (86.3") between the two second-epoch detections
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Considering the candidate 133854_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133854_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133855_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133855_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (84.2") between the two second-epoch detections
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Considering the candidate 133856_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133856_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (483.1") between the two second-epoch detections
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Considering the candidate 133861_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133861_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (587.9") between the two second-epoch detections
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Considering the candidate 133867_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133867_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (160.0") between the two second-epoch detections
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Considering the candidate 133873_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133873_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (43.0") between the two second-epoch detections
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Considering the candidate 133874_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133874_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133877_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133877_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (73.7") between the two second-epoch detections
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Considering the candidate 133884_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133884_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (726.9") between the two second-epoch detections
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Considering the candidate 133885_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133885_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (791.5") between the two second-epoch detections
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Considering the candidate 133888_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133888_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (695.9") between the two second-epoch detections
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Considering the candidate 133894_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133894_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133896_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133896_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (27.8") between the two second-epoch detections
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Considering the candidate 133897_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133897_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (41.3") between the two second-epoch detections
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Considering the candidate 133898_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133898_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (575.1") between the two second-epoch detections
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Considering the candidate 133903_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133903_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133909_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133909_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (152.8") between the two second-epoch detections
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Considering the candidate 133911_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133911_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (553.3") between the two second-epoch detections
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Considering the candidate 133916_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133916_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (473.1") between the two second-epoch detections
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Considering the candidate 133918_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133918_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (534.4") between the two second-epoch detections
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Considering the candidate 133922_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133922_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133923_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133923_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (594.8") between the two second-epoch detections
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Considering the candidate 133929_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133929_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (76.9") between the two second-epoch detections
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Considering the candidate 133931_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133931_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (761.7") between the two second-epoch detections
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Considering the candidate 133932_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133932_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (101.5") between the two second-epoch detections
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Considering the candidate 133936_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133936_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (76.8") between the two second-epoch detections
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Considering the candidate 133937_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133937_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (153.4") between the two second-epoch detections
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Considering the candidate 133938_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133938_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (210.3") between the two second-epoch detections
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Considering the candidate 133941_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133941_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (18.2") between the two second-epoch detections
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Considering the candidate 133942_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133942_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 03:34:46.89 +70:24:17.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 0.399 542828585693719552 053.69510591363 +70.40486990895 14.5351 13.5933 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.399#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133949_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133949_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (599.6") between the two second-epoch detections
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Considering the candidate 133950_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133950_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133952_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133952_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133953_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133953_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (106.9") between the two second-epoch detections
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Considering the candidate 133957_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133957_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (58.2") between the two second-epoch detections
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Considering the candidate 133958_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133958_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (83.2") between the two second-epoch detections
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Considering the candidate 133961_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133961_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133964_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133964_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (66.9") between the two second-epoch detections
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Considering the candidate 133966_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 133966_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 133967_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133967_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (652.6") between the two second-epoch detections
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Considering the candidate 133969_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133969_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (185.9") between the two second-epoch detections
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Considering the candidate 133975_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133975_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (343.2") between the two second-epoch detections
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Considering the candidate 133981_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133981_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (800.7") between the two second-epoch detections
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Considering the candidate 133991_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133991_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (675.2") between the two second-epoch detections
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Considering the candidate 133992_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133992_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (118.2") between the two second-epoch detections
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Considering the candidate 133994_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 133994_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (50.4") between the two second-epoch detections
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Considering the candidate 134010_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134010_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (650.8") between the two second-epoch detections
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Considering the candidate 134013_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134013_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (426.0") between the two second-epoch detections
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Considering the candidate 134015_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134015_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 134016_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134016_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (62.2") between the two second-epoch detections
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Considering the candidate 134023_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134023_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (24.3") between the two second-epoch detections
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Considering the candidate 134024_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134024_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (26.6") between the two second-epoch detections
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Considering the candidate 134025_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134025_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (75.1") between the two second-epoch detections
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Considering the candidate 134028_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134028_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 134029_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134029_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (727.4") between the two second-epoch detections
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Considering the candidate 134030_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134030_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (711.9") between the two second-epoch detections
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Considering the candidate 134033_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134033_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (537.2") between the two second-epoch detections
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Considering the candidate 134038_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134038_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 134040_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134040_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 134041_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134041_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (555.8") between the two second-epoch detections
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Considering the candidate 134044_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134044_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (9.7") between the two second-epoch detections
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Considering the candidate 134048_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134048_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (724.1") between the two second-epoch detections
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Considering the candidate 134054_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134054_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
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Considering the candidate 134055_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134055_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 03:34:48.31 +68:14:13.0 in the exclusion list exclusion_list.txt ****
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Considering the candidate 134056_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134056_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 134061_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134061_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 134070_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134070_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 134071_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134071_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (416.3") between the two second-epoch detections
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Considering the candidate 134072_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134072_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (730.7") between the two second-epoch detections
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Considering the candidate 134073_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134073_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (705.0") between the two second-epoch detections
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Considering the candidate 134076_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134076_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (18.0") between the two second-epoch detections
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Considering the candidate 134078_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134078_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 134081_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134081_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (179.0") between the two second-epoch detections
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Considering the candidate 134087_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134087_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (152.7") between the two second-epoch detections
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Considering the candidate 134088_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134088_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (366.6") between the two second-epoch detections
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Considering the candidate 134096_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134096_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (16.5") between the two second-epoch detections
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Considering the candidate 134097_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134097_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 134098_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134098_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (701.6") between the two second-epoch detections
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Considering the candidate 134101_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134101_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (55.1") between the two second-epoch detections
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Considering the candidate 134104_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134104_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (569.0") between the two second-epoch detections
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Considering the candidate 134105_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134105_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 134115_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134115_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (83.8") between the two second-epoch detections
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Considering the candidate 134125_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134125_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (29.9") between the two second-epoch detections
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Considering the candidate 134133_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134133_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 134136_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134136_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (617.0") between the two second-epoch detections
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Considering the candidate 134137_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134137_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (257.0") between the two second-epoch detections
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Considering the candidate 134138_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134138_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (198.7") between the two second-epoch detections
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Considering the candidate 134142_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134142_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (37.3") between the two second-epoch detections
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Considering the candidate 134143_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134143_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 134145_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134145_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
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Considering the candidate 134147_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134147_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (394.1") between the two second-epoch detections
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Considering the candidate 134159_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134159_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (88.4") between the two second-epoch detections
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Considering the candidate 134162_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134162_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 03:36:02.86 +71:29:42.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.59, MAG_FAINT_SEARCH_LIMIT=14.57)GAIADR2_OUTPUT=# 0.998 542960217850949760 054.01167925355 +71.49478863471 14.5652 13.8280 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.998#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 134166_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134166_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (614.8") between the two second-epoch detections
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Considering the candidate 134167_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134167_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134168_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134168_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134169_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134169_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134171_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134171_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134172_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134172_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (138.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134175_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134175_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (34.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134182_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134182_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (363.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134189_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134189_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (112.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134190_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134190_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (368.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134194_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134194_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (378.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134204_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134204_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134205_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134205_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 04:02:25.89 +66:01:50.4 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134210_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134210_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (600.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134213_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134213_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (152.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134215_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134215_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134224_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134224_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134228_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134228_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134232_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
Preparing report for the candidate 134232_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134238_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134238_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (321.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134239_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134239_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 03:41:48.81 +67:57:52.0 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134242_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134242_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (577.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134245_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134245_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (9.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134247_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134247_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (127.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134248_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134248_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (542.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134276_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 134276_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (604.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 77457_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 77457_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 03:41:03.85 +67:38:51.5 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 90043_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 90043_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
**** FOUND 04:05:39.23 +66:19:59.3 in the exclusion list exclusion_list.txt ****
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 62200_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212
The candidate 62200_fd_Cam-06-Q1b1x1_2026-02-21_23-24-13_20.00sec_-14.90C_LIGHT_0212 did not pass the final checks
Rejecting candidate due to large distance (210.2") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 12s
make_report_in_HTML.sh TOTAL: 192s
Prepared the HTML report for the field Cam-06-Q1b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:22:07.89 +70:28:12.0
04:11:43.24 +72:22:00.2
03:30:26.93 +72:12:32.3
04:24:10.41 +70:35:43.5
04:06:36.98 +68:36:18.0
03:34:12.73 +68:05:38.8
03:33:14.42 +73:11:24.6
03:40:05.95 +66:51:06.2
03:44:34.02 +72:43:45.9
04:07:04.74 +71:00:54.0
04:21:55.21 +72:14:51.9
03:37:07.46 +75:03:28.5
03:36:06.27 +74:10:08.1
03:47:56.15 +67:53:18.8
03:44:24.30 +67:06:02.1
04:17:40.79 +73:11:40.6
03:58:02.50 +65:53:36.7
03:55:21.70 +67:27:31.8
03:44:23.74 +69:26:47.6
03:45:20.81 +72:59:30.3
03:37:21.19 +68:07:11.7
03:37:30.19 +73:05:58.2
03:47:19.19 +68:48:45.6
03:45:42.61 +66:24:56.9
04:13:48.34 +71:34:09.3
03:35:17.32 +68:00:58.3
03:45:33.34 +73:23:58.5
04:12:16.14 +73:13:02.7
03:41:55.86 +68:36:21.9
03:41:46.99 +74:26:29.0
03:33:51.02 +73:27:45.7
03:33:48.89 +67:50:05.6
03:46:42.92 +68:52:25.6
03:53:08.08 +73:08:36.5
03:53:53.89 +71:11:44.6
04:05:44.83 +75:02:47.8
03:32:08.02 +69:08:21.9
03:52:15.61 +70:37:25.1
03:41:17.35 +68:48:39.3
03:53:27.59 +67:28:22.1
03:29:14.31 +73:23:41.4
04:01:43.33 +71:19:26.2
03:34:02.50 +70:34:00.4
03:37:42.95 +74:38:57.9
03:49:06.60 +65:09:29.1
03:47:17.36 +72:57:36.9
04:24:56.33 +71:25:51.5
03:27:27.77 +69:26:12.1
03:40:12.87 +71:31:30.6
03:57:21.93 +72:37:57.8
03:49:29.69 +69:01:42.1
03:35:58.63 +69:09:52.1
03:47:15.21 +66:33:58.4
03:32:05.72 +73:26:20.0
03:30:12.28 +70:22:44.4
03:40:42.61 +72:13:18.2
03:48:18.46 +69:46:49.7
03:43:51.78 +74:14:46.2
04:17:23.69 +72:57:04.0
03:38:08.92 +71:58:09.3
03:41:03.55 +70:03:53.1
03:49:42.41 +67:23:18.1
03:40:40.64 +69:17:39.8
03:46:35.04 +67:41:58.0
03:32:51.59 +74:13:55.9
03:36:58.79 +69:03:32.9
03:41:25.58 +68:24:24.3
03:38:29.72 +66:47:58.3
03:34:41.16 +72:06:53.7
03:52:43.90 +73:25:45.1
03:38:24.67 +68:37:37.8
########### Completed Cam-06-Q1b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ1.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
04:22:07.89 +70:28:12.0
04:11:43.24 +72:22:00.2
03:30:26.93 +72:12:32.3
04:24:10.41 +70:35:43.5
04:06:36.98 +68:36:18.0
03:34:12.73 +68:05:38.8
03:33:14.42 +73:11:24.6
03:40:05.95 +66:51:06.2
03:44:34.02 +72:43:45.9
04:07:04.74 +71:00:54.0
04:21:55.21 +72:14:51.9
03:37:07.46 +75:03:28.5
03:36:06.27 +74:10:08.1
03:47:56.15 +67:53:18.8
03:44:24.30 +67:06:02.1
04:17:40.79 +73:11:40.6
03:58:02.50 +65:53:36.7
03:55:21.70 +67:27:31.8
03:44:23.74 +69:26:47.6
03:45:20.81 +72:59:30.3
03:37:21.19 +68:07:11.7
03:37:30.19 +73:05:58.2
03:47:19.19 +68:48:45.6
03:45:42.61 +66:24:56.9
04:13:48.34 +71:34:09.3
03:35:17.32 +68:00:58.3
03:45:33.34 +73:23:58.5
04:12:16.14 +73:13:02.7
03:41:55.86 +68:36:21.9
03:41:46.99 +74:26:29.0
03:33:51.02 +73:27:45.7
03:33:48.89 +67:50:05.6
03:46:42.92 +68:52:25.6
03:53:08.08 +73:08:36.5
03:53:53.89 +71:11:44.6
04:05:44.83 +75:02:47.8
03:32:08.02 +69:08:21.9
03:52:15.61 +70:37:25.1
03:41:17.35 +68:48:39.3
03:53:27.59 +67:28:22.1
03:29:14.31 +73:23:41.4
04:01:43.33 +71:19:26.2
03:34:02.50 +70:34:00.4
03:37:42.95 +74:38:57.9
03:49:06.60 +65:09:29.1
03:47:17.36 +72:57:36.9
04:24:56.33 +71:25:51.5
03:27:27.77 +69:26:12.1
03:40:12.87 +71:31:30.6
03:57:21.93 +72:37:57.8
03:49:29.69 +69:01:42.1
03:35:58.63 +69:09:52.1
03:47:15.21 +66:33:58.4
03:32:05.72 +73:26:20.0
03:30:12.28 +70:22:44.4
03:40:42.61 +72:13:18.2
03:48:18.46 +69:46:49.7
03:43:51.78 +74:14:46.2
04:17:23.69 +72:57:04.0
03:38:08.92 +71:58:09.3
03:41:03.55 +70:03:53.1
03:49:42.41 +67:23:18.1
03:40:40.64 +69:17:39.8
03:46:35.04 +67:41:58.0
03:32:51.59 +74:13:55.9
03:36:58.79 +69:03:32.9
03:41:25.58 +68:24:24.3
03:38:29.72 +66:47:58.3
03:34:41.16 +72:06:53.7
03:52:43.90 +73:25:45.1
03:38:24.67 +68:37:37.8
###################################################################################
04:22:07.89 +70:28:12.0 -- not an asteroid (will add it to exclusion list)
04:11:43.24 +72:22:00.2 -- not an asteroid (will add it to exclusion list)
03:30:26.93 +72:12:32.3 -- not an asteroid (will add it to exclusion list)
04:24:10.41 +70:35:43.5 -- not an asteroid (will add it to exclusion list)
04:06:36.98 +68:36:18.0 -- not an asteroid (will add it to exclusion list)
03:34:12.73 +68:05:38.8 -- not an asteroid (will add it to exclusion list)
03:33:14.42 +73:11:24.6 -- not an asteroid (will add it to exclusion list)
03:40:05.95 +66:51:06.2 -- not an asteroid (will add it to exclusion list)
03:44:34.02 +72:43:45.9 -- not an asteroid (will add it to exclusion list)
04:07:04.74 +71:00:54.0 -- not an asteroid (will add it to exclusion list)
04:21:55.21 +72:14:51.9 -- not an asteroid (will add it to exclusion list)
03:37:07.46 +75:03:28.5 -- not an asteroid (will add it to exclusion list)
03:36:06.27 +74:10:08.1 -- not an asteroid (will add it to exclusion list)
03:47:56.15 +67:53:18.8 -- not an asteroid (will add it to exclusion list)
03:44:24.30 +67:06:02.1 -- not an asteroid (will add it to exclusion list)
04:17:40.79 +73:11:40.6 -- not an asteroid (will add it to exclusion list)
03:58:02.50 +65:53:36.7 -- not an asteroid (will add it to exclusion list)
03:55:21.70 +67:27:31.8 -- not an asteroid (will add it to exclusion list)
03:44:23.74 +69:26:47.6 -- not an asteroid (will add it to exclusion list)
03:45:20.81 +72:59:30.3 -- not an asteroid (will add it to exclusion list)
03:37:21.19 +68:07:11.7 -- not an asteroid (will add it to exclusion list)
03:37:30.19 +73:05:58.2 -- not an asteroid (will add it to exclusion list)
03:47:19.19 +68:48:45.6 -- not an asteroid (will add it to exclusion list)
03:45:42.61 +66:24:56.9 -- not an asteroid (will add it to exclusion list)
04:13:48.34 +71:34:09.3 -- not an asteroid (will add it to exclusion list)
03:35:17.32 +68:00:58.3 -- not an asteroid (will add it to exclusion list)
03:45:33.34 +73:23:58.5 -- not an asteroid (will add it to exclusion list)
04:12:16.14 +73:13:02.7 -- not an asteroid (will add it to exclusion list)
03:41:55.86 +68:36:21.9 -- not an asteroid (will add it to exclusion list)
03:41:46.99 +74:26:29.0 -- not an asteroid (will add it to exclusion list)
03:33:51.02 +73:27:45.7 -- not an asteroid (will add it to exclusion list)
03:33:48.89 +67:50:05.6 -- not an asteroid (will add it to exclusion list)
03:46:42.92 +68:52:25.6 -- not an asteroid (will add it to exclusion list)
03:53:08.08 +73:08:36.5 -- not an asteroid (will add it to exclusion list)
03:53:53.89 +71:11:44.6 -- not an asteroid (will add it to exclusion list)
04:05:44.83 +75:02:47.8 -- not an asteroid (will add it to exclusion list)
03:32:08.02 +69:08:21.9 -- not an asteroid (will add it to exclusion list)
03:52:15.61 +70:37:25.1 -- not an asteroid (will add it to exclusion list)
03:41:17.35 +68:48:39.3 -- not an asteroid (will add it to exclusion list)
03:53:27.59 +67:28:22.1 -- not an asteroid (will add it to exclusion list)
03:29:14.31 +73:23:41.4 -- not an asteroid (will add it to exclusion list)
04:01:43.33 +71:19:26.2 -- not an asteroid (will add it to exclusion list)
03:34:02.50 +70:34:00.4 -- not an asteroid (will add it to exclusion list)
03:37:42.95 +74:38:57.9 -- not an asteroid (will add it to exclusion list)
03:49:06.60 +65:09:29.1 -- not an asteroid (will add it to exclusion list)
03:47:17.36 +72:57:36.9 -- not an asteroid (will add it to exclusion list)
04:24:56.33 +71:25:51.5 -- not an asteroid (will add it to exclusion list)
03:27:27.77 +69:26:12.1 -- not an asteroid (will add it to exclusion list)
03:40:12.87 +71:31:30.6 -- not an asteroid (will add it to exclusion list)
03:57:21.93 +72:37:57.8 -- not an asteroid (will add it to exclusion list)
03:49:29.69 +69:01:42.1 -- not an asteroid (will add it to exclusion list)
03:35:58.63 +69:09:52.1 -- not an asteroid (will add it to exclusion list)
03:47:15.21 +66:33:58.4 -- not an asteroid (will add it to exclusion list)
03:32:05.72 +73:26:20.0 -- not an asteroid (will add it to exclusion list)
03:30:12.28 +70:22:44.4 -- not an asteroid (will add it to exclusion list)
03:40:42.61 +72:13:18.2 -- not an asteroid (will add it to exclusion list)
03:48:18.46 +69:46:49.7 -- not an asteroid (will add it to exclusion list)
03:43:51.78 +74:14:46.2 -- not an asteroid (will add it to exclusion list)
04:17:23.69 +72:57:04.0 -- not an asteroid (will add it to exclusion list)
03:38:08.92 +71:58:09.3 -- not an asteroid (will add it to exclusion list)
03:41:03.55 +70:03:53.1 -- not an asteroid (will add it to exclusion list)
03:49:42.41 +67:23:18.1 -- not an asteroid (will add it to exclusion list)
03:40:40.64 +69:17:39.8 -- not an asteroid (will add it to exclusion list)
03:46:35.04 +67:41:58.0 -- not an asteroid (will add it to exclusion list)
03:32:51.59 +74:13:55.9 -- not an asteroid (will add it to exclusion list)
03:36:58.79 +69:03:32.9 -- not an asteroid (will add it to exclusion list)
03:41:25.58 +68:24:24.3 -- not an asteroid (will add it to exclusion list)
03:38:29.72 +66:47:58.3 -- not an asteroid (will add it to exclusion list)
03:34:41.16 +72:06:53.7 -- not an asteroid (will add it to exclusion list)
03:52:43.90 +73:25:45.1 -- not an asteroid (will add it to exclusion list)
03:38:24.67 +68:37:37.8 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
03:27:27.77 +69:26:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:29:14.31 +73:23:41.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:30:12.28 +70:22:44.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:30:26.93 +72:12:32.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:32:05.72 +73:26:20.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:32:08.02 +69:08:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:32:51.59 +74:13:55.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:33:14.42 +73:11:24.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:33:48.89 +67:50:05.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:33:51.02 +73:27:45.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:02.50 +70:34:00.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:12.73 +68:05:38.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:34:41.16 +72:06:53.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:17.32 +68:00:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:35:58.63 +69:09:52.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:06.27 +74:10:08.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:36:58.79 +69:03:32.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:07.46 +75:03:28.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:21.19 +68:07:11.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:30.19 +73:05:58.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:37:42.95 +74:38:57.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:08.92 +71:58:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:24.67 +68:37:37.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:38:29.72 +66:47:58.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:05.95 +66:51:06.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:12.87 +71:31:30.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:40.64 +69:17:39.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:40:42.61 +72:13:18.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:03.55 +70:03:53.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:17.35 +68:48:39.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:25.58 +68:24:24.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:46.99 +74:26:29.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:55.86 +68:36:21.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:43:51.78 +74:14:46.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:23.74 +69:26:47.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:24.30 +67:06:02.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:34.02 +72:43:45.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:20.81 +72:59:30.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:33.34 +73:23:58.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:45:42.61 +66:24:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:35.04 +67:41:58.0 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:42.92 +68:52:25.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:15.21 +66:33:58.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:17.36 +72:57:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:19.19 +68:48:45.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:47:56.15 +67:53:18.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:48:18.46 +69:46:49.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:06.60 +65:09:29.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:29.69 +69:01:42.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:42.41 +67:23:18.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:15.61 +70:37:25.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:52:43.90 +73:25:45.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:08.08 +73:08:36.5 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:27.59 +67:28:22.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:53.89 +71:11:44.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:55:21.70 +67:27:31.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:57:21.93 +72:37:57.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:58:02.50 +65:53:36.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:01:43.33 +71:19:26.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:05:44.83 +75:02:47.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:06:36.98 +68:36:18.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:07:04.74 +71:00:54.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:11:43.24 +72:22:00.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:12:16.14 +73:13:02.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:13:48.34 +71:34:09.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:17:23.69 +72:57:04.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:17:40.79 +73:11:40.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:21:55.21 +72:14:51.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:22:07.89 +70:28:12.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:10.41 +70:35:43.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:56.33 +71:25:51.5 -- 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)
03:27:27.77 +69:26:12.1 -- not a known variable star
03:29:14.31 +73:23:41.4 -- not a known variable star
03:30:12.28 +70:22:44.4 -- not a known variable star
03:30:26.93 +72:12:32.3 -- not a known variable star
03:32:05.72 +73:26:20.0 -- not a known variable star
03:32:08.02 +69:08:21.9 -- not a known variable star
03:32:51.59 +74:13:55.9 -- a known variable star
03:33:14.42 +73:11:24.6 -- not a known variable star
03:33:48.89 +67:50:05.6 -- not a known variable star
03:33:51.02 +73:27:45.7 -- not a known variable star
03:34:02.50 +70:34:00.4 -- not a known variable star
03:34:12.73 +68:05:38.8 -- a known variable star
03:34:41.16 +72:06:53.7 -- not a known variable star
03:35:17.32 +68:00:58.3 -- not a known variable star
03:35:58.63 +69:09:52.1 -- not a known variable star
03:36:06.27 +74:10:08.1 -- not a known variable star
03:36:58.79 +69:03:32.9 -- a known variable star
03:37:07.46 +75:03:28.5 -- not a known variable star
03:37:21.19 +68:07:11.7 -- not a known variable star
03:37:30.19 +73:05:58.2 -- not a known variable star
03:37:42.95 +74:38:57.9 -- not a known variable star
03:38:08.92 +71:58:09.3 -- not a known variable star
03:38:24.67 +68:37:37.8 -- a known variable star
03:38:29.72 +66:47:58.3 -- not a known variable star
03:40:05.95 +66:51:06.2 -- not a known variable star
03:40:12.87 +71:31:30.6 -- not a known variable star
03:40:40.64 +69:17:39.8 -- a known variable star
03:40:42.61 +72:13:18.2 -- not a known variable star
03:41:03.55 +70:03:53.1 -- a known variable star
03:41:17.35 +68:48:39.3 -- not a known variable star
03:41:25.58 +68:24:24.3 -- not a known variable star
03:41:46.99 +74:26:29.0 -- not a known variable star
03:41:55.86 +68:36:21.9 -- not a known variable star
03:43:51.78 +74:14:46.2 -- not a known variable star
03:44:23.74 +69:26:47.6 -- not a known variable star
03:44:24.30 +67:06:02.1 -- not a known variable star
03:44:34.02 +72:43:45.9 -- a known variable star
03:45:20.81 +72:59:30.3 -- not a known variable star
03:45:33.34 +73:23:58.5 -- not a known variable star
03:45:42.61 +66:24:56.9 -- not a known variable star
03:46:35.04 +67:41:58.0 -- not a known variable star
03:46:42.92 +68:52:25.6 -- not a known variable star
03:47:15.21 +66:33:58.4 -- not a known variable star
03:47:17.36 +72:57:36.9 -- not a known variable star
03:47:19.19 +68:48:45.6 -- not a known variable star
03:47:56.15 +67:53:18.8 -- not a known variable star
03:48:18.46 +69:46:49.7 -- a known variable star
03:49:06.60 +65:09:29.1 -- not a known variable star
03:49:29.69 +69:01:42.1 -- not a known variable star
03:49:42.41 +67:23:18.1 -- not a known variable star
03:52:15.61 +70:37:25.1 -- not a known variable star
03:52:43.90 +73:25:45.1 -- not a known variable star
03:53:08.08 +73:08:36.5 -- not a known variable star
03:53:27.59 +67:28:22.1 -- not a known variable star
03:53:53.89 +71:11:44.6 -- not a known variable star
03:55:21.70 +67:27:31.8 -- not a known variable star
03:57:21.93 +72:37:57.8 -- a known variable star
03:58:02.50 +65:53:36.7 -- not a known variable star
04:01:43.33 +71:19:26.2 -- a known variable star
04:05:44.83 +75:02:47.8 -- not a known variable star
04:06:36.98 +68:36:18.0 -- not a known variable star
04:07:04.74 +71:00:54.0 -- not a known variable star
04:11:43.24 +72:22:00.2 -- not a known variable star
04:12:16.14 +73:13:02.7 -- not a known variable star
04:13:48.34 +71:34:09.3 -- not a known variable star
04:17:23.69 +72:57:04.0 -- not a known variable star
04:17:40.79 +73:11:40.6 -- not a known variable star
04:21:55.21 +72:14:51.9 -- not a known variable star
04:22:07.89 +70:28:12.0 -- not a known variable star
04:24:10.41 +70:35:43.5 -- not a known variable star
04:24:56.33 +71:25:51.5 -- not a known variable star
Found 61 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
71 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 71 (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)2461093.72475690 -observatory 500
23:23:32.92 -01:57:11.5 Mercury (-0.1mag)
23:04:43.70 -07:28:09.2 Venus (-3.9mag)
21:42:59.24 -14:51:57.6 Mars (1.1mag)
07:06:05.21 +22:54:21.5 Jupiter (-2.5mag)
00:05:27.62 -01:44:18.4 Saturn (1.0mag)
03:39:59.72 +19:21:44.5 Uranus (5.7mag)
00:03:41.32 -01:01:34.5 Neptune (7.8mag)
20:29:07.47 -22:59:33.2 Pluto (14.5mag)
01:57:18.69 +16:34:26.7 Moon (-9.6mag)
-rw-r--r-- 1 apache apache 362 Feb 22 02:38 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461093.72475690:
07:06:11.01 +22:54:12.3 Io (5.4mag)
07:06:17.59 +22:53:58.3 Europa (5.5mag)
07:05:57.30 +22:54:44.8 Ganymede (4.9mag)
07:06:25.16 +22:53:54.2 Callisto (6.2mag)
07:09:14.45 +23:10:42.8 Himalia (15.0mag)
07:06:08.66 +22:54:16.5 Thebe (15.9mag)
07:08:39.48 +23:19:13.6 Elara (17.0mag)
07:01:38.95 +24:02:17.8 Pasiphae (17.0mag)
07:15:06.09 +22:42:22.6 Carme (18.1mag)
00:05:39.38 -01:44:22.8 Titan (8.8mag)
00:05:33.23 -01:44:16.9 Rhea (10.1mag)
00:05:23.17 -01:45:39.0 Iapetus (11.5mag)
00:05:28.70 -01:44:21.7 Hyperion (14.8mag)
00:07:31.88 -01:31:18.6 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Feb 22 02:38 moons.txt
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Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461093.72475690:
08:46:19.73 +24:30:46.7 JWST
12:59:05.24 +53:29:03.4 Chandra
16:11:58.22 -54:38:45.5 XMM-Newton
-rw-r--r-- 1 apache apache 96 Feb 22 02:38 spacecraft.txt
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Positions of bright comets (listed at http://astro.vanbuitenen.nl/comets and http://aerith.net/comet/weekly/current.html ) from JPL HORIZONS for JD(UT)2461093.72475690 at 500
16:59:49.77 -11:03:52.5 17.5mag 10P/Tempel 2
03:37:22.81 +28:58:04.0 18.0mag 123P/West-Hartley
08:23:32.13 +60:41:37.4 18.4mag 124P/Mrkos
21:19:48.58 -07:37:36.7 22.1mag 141P/Machholz
01:21:18.29 +11:56:02.3 17.7mag 145P/Shoemaker-Levy 5
11:02:55.01 +30:35:00.6 17.9mag 164P/Christensen
09:33:05.62 -33:51:37.0 18.0mag 195P/Hill
15:52:02.78 -06:35:29.0 19.2mag 210P/Christensen
18:17:11.04 -21:28:16.0 17.3mag 218P/LINEAR
16:21:41.30 -18:10:50.2 15.2mag 235P/LINEAR
03:56:29.38 +27:45:17.1 17.8mag 240P/NEAT
15:17:42.79 +06:38:06.1 14.8mag 24P/Schaumasse
11:23:29.37 -03:23:03.1 17.4mag 29P/Schwassmann-Wachmann 1
07:03:47.33 +27:24:51.4 19.6mag 407P/PanSTARRS-Fuls
17:07:15.75 -11:19:12.3 17.6mag 40P/Vaisala 1
11:02:10.12 -08:51:38.6 16.6mag 43P/Wolf-Harrington
13:25:29.99 -05:49:52.6 20.0mag 489P/Denning
04:34:25.27 +48:34:13.2 17.8mag 493P/2024 Q2 (LONEOS)
06:04:24.86 +47:30:40.5 17.7mag 63P/Wild 1
23:14:44.94 -02:06:44.2 16.2mag 78P/Gehrels 2
20:01:46.15 -22:17:41.0 14.9mag 88P/Howell
15:27:56.78 -29:01:01.1 18.7mag P/2023 S1 (PanSTARRS)
04:43:27.53 -72:35:39.6 16.5mag C/2014 UN271 (Bernardinelli-Bernstein)
05:29:49.37 +31:12:54.9 18.2mag C/2017 K2 (PanSTARRS)
20:06:40.62 -65:11:46.2 18.1mag C/2020 V2 (ZTF)
17:21:42.21 +04:21:49.8 16.3mag C/2021 G2 (ATLAS)
03:35:44.43 +24:36:47.4 15.8mag C/2022 N2 (PanSTARRS)
09:08:11.77 +29:49:55.3 15.3mag C/2022 QE78 (ATLAS)
08:35:39.26 -06:33:15.3 16.7mag C/2022 R6 (PanSTARRS)
23:53:07.56 +48:26:56.0 18.0mag C/2023 C2 (ATLAS)
09:51:03.09 -20:45:21.7 17.5mag C/2023 F3 (ATLAS)
20:34:53.89 +61:14:31.2 17.3mag C/2023 H5 (Lemmon)
19:34:30.63 -03:24:18.0 16.1mag C/2023 R1 (PANSTARRS)
02:48:56.74 +35:40:32.2 18.5mag C/2023 RS61 (PanSTARRS)
21:01:34.28 +81:20:02.0 18.0mag C/2023 X2 (Lemmon)
06:39:03.49 +63:49:19.4 17.3mag C/2024 A1 (ATLAS)
01:57:16.99 -24:31:53.7 11.2mag C/2024 E1 (Wierzchos)
11:44:55.29 -02:34:01.9 18.1mag C/2024 G2 (ATLAS)
19:28:23.14 +00:39:21.3 19.0mag C/2024 G4 (PanSTARRS)
16:37:11.60 -01:42:19.0 17.7mag C/2024 G6 (ATLAS)
19:53:30.57 +03:15:54.5 15.6mag C/2024 J3 (ATLAS)
02:47:16.90 -31:33:39.6 15.4mag C/2024 T5 (ATLAS)
16:24:54.22 -58:15:29.4 15.6mag C/2025 A6 (Lemmon)
04:50:28.65 +62:12:47.9 16.7mag C/2025 J1 (Borisov)
00:00:00.00 +00:00:00.0 cannot get JPL HORIZONS ephemerides for non-periodic comet C/2025 K1 (ATLAS)
15:56:40.43 -12:57:40.6 14.8mag C/2025 L1 (ATLAS)
02:20:17.77 -19:06:34.7 16.7mag C/2025 Q3 (ATLAS)
02:09:40.05 +17:17:08.8 21.2mag C/2025 R2 (SWAN)
22:20:47.43 +17:39:20.9 16.4mag C/2025 R3 (PANSTARRS)
21:46:05.86 -16:51:20.5 21.5mag C/2025 T1 (ATLAS)
03:06:04.49 -20:31:55.5 18.3mag C/2026 A1 (MAPS)
21:03:18.22 +20:57:35.5 16.9mag C/2026 B2 (Sun-Gao)
-rw-r--r-- 1 apache apache 2.6K Feb 22 02:39 comets.txt
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List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
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
13:01:07.08 -11:25:16.30 AT2026bzh 2026-02-12.45 17.3
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
06:30:51.72 -74:35:50.10 AT2026ahr 2026-01-20.19 17.09
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:24.99 +04:00:02.20 SN 2026kc 2026-01-18.61 16.1
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
03:36:21.80 -31:44:39.30 AT2025aibn 2026-01-17.04 16.7
13:45:00.71 -32:34:53.00 AT2026yi 2026-01-17.26 16.22
09:27:07.17 +62:45:24.20 AT2026nu 2026-01-17.29 17.09
12:38:41.73 +07:36:37.40 SN 2025afcr 2026-01-17.49 17.11
12:12:12.65 +13:13:18.50 SN 2026acd 2026-01-17.3 16.15
16:21:54.73 -63:36:53.10 ASASSN-26al 2026-01-17.36 15.34
15:33:45.22 -22:11:07.90 ASASSN-26aj 2026-01-16.51 14
12:27:08.33 -58:19:36.10 ASASSN-26ak 2026-01-16.2 13.94
17:21:53.10 +04:39:07.10 ASASSN-26ai 2026-01-16.67 14.83
14:46:54.08 -64:04:30.10 ASASSN-26ah 2026-01-15.07 16.84
23:02:43.24 +20:04:53.00 SN2025ajvh 2026-01-15.07 16.03
14:12:27.38 -30:12:29.10 ASASSN-26ag 2026-01-14.27 15.35
14:33:53.58 +05:27:35.40 SN 2025ajnc 2026-01-14.32 15.79
01:43:00.31 -34:11:40.60 AT2025afcm 2026-01-13.08 0.45
00:26:17.71 -52:11:38.60 AT2025ahal 2026-01-11.06 17.57
00:51:36.17 +29:42:40.10 SN2025ahxd 2026-01-11.21 15
10:19:19.14 -37:54:58.30 AT2025ahrt 2026-01-10.26 -0.54
14:37:48.78 +15:51:04.20 SN2025ajng 2026-01-9.42 16.35
05:01:03.70 -08:34:13.20 SN2026A 2026-01-9.28 16.83
00:02:52.11 +13:05:42.90 SN2025ajvg 2026-01-9.13 15.89
08:37:09.62 -02:18:08.80 SN2025aigm 2026-01-9.55 17.66
09:52:50.71 +39:36:55.70 SN2025ahyt 2026-01-9.37 16.97
11:22:19.08 -27:21:40.90 AT2026ta 2026-01-9.32 15.88
14:35:00.21 +00:59:11.40 SN 2025ahsa 2026-01-8.35 -2
09:25:42.42 +22:20:06.10 SN2025ahkt 2026-01-8.03 15.88
22:39:53.44 +34:53:50.00 SN 2025aikz 2026-01-7.09 16.3
08:21:20.95 +20:52:01.60 SN 2025aiks 2026-01-7.13 15.82
07:35:31.38 +09:10:32.40 AT2025ajvk 2026-01-7.12 -1.82
02:50:07.71 -16:37:02.30 AT2026nl 2026-01-7.16 14.19
14:05:12.75 -33:46:00.80 SN 2025ajmj 2026-01-7.31 14.93
12:35:08.33 +28:03:22.70 SN 2025aiaj 2026-01-5.44 15.76
05:30:00.47 -66:43:29.40 ASASSN-26af 2026-01-5.12 14.38
14:05:05.13 -44:14:24.00 ASASSN-26ac 2026-01-5.3 16.01
11:29:16.57 +20:35:09.00 AT2025alco 2026-01-4.39 15.93
16:42:59.28 +26:21:02.80 ASASSN-26ae 2026-01-4.52 14.31
04:13:46.60 -05:02:16.60 ASASSN-26ad 2026-01-4.32 14.58
05:00:01.32 -57:14:29.70 ASASSN-25fj/ASASSN-26ab 2026-01-1.19 13.38
13:53:51.35 -17:55:38.10 ASASSN-25fg 2025-12-23.33 16.66
06:18:15.27 +15:47:38.10 AT2025ahtd 2025-12-23.31 16.96
07:20:53.12 -33:02:58.20 SN 2025agvw 2025-12-23.32 16.84
02:58:15.63 +44:47:45.80 ASASSN-25fh 2025-12-23.13 15.63
04:51:03.78 -36:13:59.00 AT2025aftm 2025-12-20.14 17.35
03:12:59.31 +17:41:45.20 SN2025afzm 2025-12-20.15 17.22
13:33:14.27 -46:03:33.90 ASASSN-25fc 2025-12-19.32 SDSS
07:07:30.84 +24:37:55.60 SN2025agie 2025-12-19.19 16.96
12:31:24.34 -59:07:09.00 ASASSN-25fd 2025-12-19.06 14.94
14:02:20.59 -20:28:28.70 ASASSN-25fe 2025-12-19.34 SDSS
08:08:51.65 -16:39:31.50 ASASSN-25ff 2025-12-19.22 SDSS
00:34:05.69 +05:21:07.50 SN2025afty 2025-12-18.21 16.92
01:35:25.55 -05:40:42.00 AT2025agsf 2025-12-18.12 17.67
06:12:00.84 -46:50:40.70 AT2025aetd 2025-12-15.08 17.32
11:07:12.05 -55:12:59.00 ASASSN-25fa 2025-12-14.25 16.07
02:48:09.78 +37:45:17.90 AT2025afje 2025-12-13.28 17.65
08:17:38.99 +59:57:25.90 SN2025afcy 2025-12-13.43 16.8
22:58:25.70 +26:38:19.80 SN 2025afve 2025-12-12.1 16.63
03:44:52.10 -59:08:22.80 SN 2025aegk 2025-12-12.1 SDSS
04:55:47.45 -18:56:49.70 SN 2025aetg 2025-12-11.36 16.92
23:15:07.77 +13:10:19.80 SN 2025afwb 2025-12-11.2 17.13
02:19:39.33 -45:39:00.60 SN 2025aeqg 2025-12-10.07 16.77
02:03:03.89 +04:14:37.30 SN2025afih 2025-12-8.1 16.49
22:23:03.49 -56:35:57.50 AT2025aeei 2025-12-8.03 16.01
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############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
14:45:58.45 +39:05:10.3 TCP J14455845+3905103 2025-12-30.8196 14.1mag
00:43:23.44 +41:24:35.7 PNV J00432344+4124357 2025-12-11.684 19.7mag
00:41:01.11 +41:59:28.2 PNV J00410111+4159282 2026-01-06.1994 18.7mag
00:42:52.01 +41:14:29.2 PNV J00425201+4114292 2026-01-08.7863 18.37Cmag
02:50:07.72 -16:37:02.3 TCP J02500772-1637023 2026-01-06.6352 14.53Cmag
00:42:58.52 +41:14:44.2 PNV J00425852+4114442 2026-01-13.4991 16.89Cmag
14:47:33.95 -10:02:56.8 TCP J14473395-1002568 2026-01-13.8185 14.0mag
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
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
-rw-r--r-- 1 apache apache 187K Feb 22 02:38 tocp_transients_list.txt
