This analysis is done by the script util/transients/transient_factory_test31.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx
The list of candidates will appear below. Please manually reload the page every few minutes untill the 'Processing complete' message appears.
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.55 04:49:03.90 +69:07:44.0
141.47503 15.34870 galactic Cam Second-epoch detections are separated by 2.2" and 2.1 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 | 04:49:03.90 +69:07:44.0 (user input) | T | P | (position from user input) J-Ks=0.521+/-0.038 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:49:03.90 +69:07:44.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.45 06:20:35.20 +72:57:44.3
141.41020 23.63912 galactic Cam Second-epoch detections are separated by 0.6" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:20:35.20 +72:57:44.3 (user input) | T | P | (position from user input) J-Ks=0.628+/-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,2461121.7296,13.45,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.45CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:20:35.20 +72:57:44.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.55 04:28:03.62 +70:46:00.9
138.98019 15.00218 galactic Cam Second-epoch detections are separated by 1.0" and 2.2 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 | 04:28:03.62 +70:46:00.9 (user input) | T | P | (position from user input) J-Ks=0.442+/-0.046 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:28:03.62 +70:46:00.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.47 05:15:41.24 +72:19:02.5
140.00124 18.95081 galactic Cam Second-epoch detections are separated by 1.0" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:15:41.24 +72:19:02.5 (user input) | T | P | (position from user input) J-Ks=0.282+/-0.049 (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,2461121.7296,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:15:41.24 +72:19:02.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.51 04:24:09.95 +70:35:42.9
138.88840 14.64815 galactic Cam Second-epoch detections are separated by 1.4" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:24:09.95 +70:35:42.9 (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,2461121.7296,13.51,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.51CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:09.95 +70:35:42.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.32 04:19:02.37 +69:20:47.4
139.51589 13.47284 galactic Cam Second-epoch detections are separated by 1.9" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 496892261195893120 | 04:18:54.28 +69:20:57.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 496892261195893120,2461121.7296,13.32,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 496892261195893120 20260322.2296 13.32CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:19:02.37 +69:20:47.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.48,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.48CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:20:24.98 +74:02:54.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.37 04:12:12.07 +72:09:08.5
137.04180 15.03467 galactic Cam Second-epoch detections are separated by 0.8" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:12:12.07 +72:09:08.5 (user input) | T | P | (position from user input) J-Ks=0.345+/-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,2461121.7296,13.37,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.37CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:12:12.07 +72:09:08.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:15:21.53 +66:29:41.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.00 03:50:31.20 +66:54:01.6
139.21976 9.87728 galactic Cam Second-epoch detections are separated by 1.5" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:50:31.20 +66:54:01.6 (user input) | T | P | (position from user input) J-Ks=0.376+/-0.030 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.00,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.00CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:50:31.20 +66:54:01.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,12.87,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 12.87CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:15:29.39 +66:00:07.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,12.89,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 12.89CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:01.16 +69:27:18.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.96 04:01:13.81 +67:58:11.5
139.30186 11.35784 galactic Cam Second-epoch detections are separated by 2.6" and 2.2 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 | 04:01:13.81 +67:58:11.5 (user input) | T | P | (position from user input) J-Ks=0.845+/-0.031 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,12.96,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 12.96CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:01:13.81 +67:58:11.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.93 04:11:33.42 +65:34:22.7
141.72254 10.29654 galactic Cam Second-epoch detections are separated by 0.6" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:11:33.42 +65:34:22.7 (user input) | T | P | (position from user input) J-Ks=0.554+/-0.027 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:11:33.42 +65:34:22.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 490135487366331520,2461121.7296,12.91,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 490135487366331520 20260322.2296 12.91CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:41.47 +66:34:54.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.80 06:11:29.09 +72:25:46.6
141.75147 22.83703 galactic Cam Second-epoch detections are separated by 3.3" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:11:29.09 +72:25:46.6 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,12.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 12.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:11:29.09 +72:25:46.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.83 04:32:07.01 +69:05:36.9
140.51496 14.15676 galactic Cam Second-epoch detections are separated by 0.7" and 2.5 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 | 04:32:07.01 +69:05:36.9 (user input) | T | P | (position from user input) J-Ks=0.394+/-0.038 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,12.83,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 12.83CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:32:07.01 +69:05:36.9 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.78 04:07:03.75 +71:00:40.5
137.56662 13.93534 galactic Cam Second-epoch detections are separated by 2.7" and 2.2 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 | 04:07:03.75 +71:00:40.5 (user input) | T | P | (position from user input) J-Ks=0.375+/-0.033 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,12.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 12.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:07:03.75 +71:00:40.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.76 03:41:16.99 +68:14:56.9
137.66604 10.38211 galactic Cam Second-epoch detections are separated by 0.6" and 2.2 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 | 03:41:16.99 +68:14:56.9 (user input) | T | P | (position from user input) J-Ks=0.907+/-0.028 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,12.76,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 12.76CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:41:16.99 +68:14:56.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.63 03:46:59.15 +68:04:12.3
138.20229 10.56997 galactic Cam Second-epoch detections are separated by 1.2" and 2.0 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 | 03:46:59.15 +68:04:12.3 (user input) | T | P | (position from user input) J-Ks=0.414+/-0.028 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,12.63,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 12.63CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:46:59.15 +68:04:12.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.40 03:58:42.91 +65:14:45.2
140.94728 9.15309 galactic Cam Second-epoch detections are separated by 1.0" and 2.1 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 489035529061898240 | 03:58:46.98 +65:14:55.8 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.792+/-0.026 (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 489035529061898240,2461121.7296,12.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 489035529061898240 20260322.2296 12.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:58:42.91 +65:14:45.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.09 03:55:21.86 +67:27:33.4
139.21950 10.60726 galactic Cam Second-epoch detections are separated by 1.7" and 2.2 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 | 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
CzeV3511,2461121.7296,12.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
CzeV3511 20260322.2296 12.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:55:21.86 +67:27:33.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 11.11 03:44:35.35 +68:53:12.1
137.50817 11.07030 galactic Cam Second-epoch detections are separated by 2.0" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 494414717901684096 | 03:44:31.88 +68:53:09.3 (Gaia DR3) | ROT (local) | (local) | 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 494414717901684096,2461121.7296,11.11,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 494414717901684096 20260322.2296 11.11CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:44:35.35 +68:53:12.1 ;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-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 11.31 04:00:27.59 +68:34:39.6
138.83320 11.76242 galactic Cam Second-epoch detections are separated by 1.0" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 493787098621550976 | 04:00:22.15 +68:34:24.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=1.187+/-0.050 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 493787098621550976,2461121.7296,11.31,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493787098621550976 20260322.2296 11.31CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:00:27.59 +68:34:39.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 11.94 04:26:19.36 +74:06:02.6
136.29219 17.11402 galactic Cam Second-epoch detections are separated by 1.4" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | ATO J066.5612+74.0978 | 04:26:12.95 +74:06:29.8 (Gaia DR3) | dubious (ATLAS) | (ATLAS) | Gaia3var=NOT_AVAILABLE J-Ks=0.518+/-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
ATO J066.5612+74.0978,2461121.7296,11.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
ATO J066.5612+74.0978 20260322.2296 11.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:26:19.36 +74:06:02.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.05 03:37:03.62 +69:30:34.3
136.58115 11.15496 galactic Cas Second-epoch detections are separated by 1.1" and 2.4 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 03:37:03.62 +69:30:34.3 (user input) | T | P | (position from user input) J-Ks=0.280+/-0.033 (F)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
TCP 2026 03 22.2295* 03 37 03.62 +69 30 34.3 12.1 U Cas 9 0
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,12.05,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 12.05CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:37:03.62 +69:30:34.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.21 03:49:46.61 +66:14:44.9
139.58324 9.32450 galactic Cam Second-epoch detections are separated by 0.9" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 490079549712449664 | 03:49:39.59 +66:14:46.3 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.933+/-0.027 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 490079549712449664,2461121.7296,12.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 490079549712449664 20260322.2296 12.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:49:46.61 +66:14:44.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.53 03:58:19.27 +68:28:27.8
138.75392 11.55519 galactic Cam Second-epoch detections are separated by 2.7" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 493779608198576640 | 03:58:15.05 +68:28:25.0 (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 493779608198576640,2461121.7296,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493779608198576640 20260322.2296 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:58:19.27 +68:28:27.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.59 03:57:23.68 +71:25:00.8
136.69425 13.70595 galactic Cam Second-epoch detections are separated by 0.5" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 495284156721043456 | 03:57:27.88 +71:25:33.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.466+/-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 495284156721043456,2461121.7296,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 495284156721043456 20260322.2296 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:57:23.68 +71:25:00.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.59 04:27:03.91 +67:43:40.8
141.24372 12.90036 galactic Cam Second-epoch detections are separated by 1.9" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 495750452730515584 | 04:27:00.65 +67:43:23.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.898+/-0.033 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 495750452730515584,2461121.7296,12.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 495750452730515584 20260322.2296 12.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:27:03.91 +67:43:40.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.55 04:50:31.21 +70:07:14.5
140.73305 16.04833 galactic Cam Second-epoch detections are separated by 0.9" and 2.4 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 | 04:50:31.21 +70:07:14.5 (user input) | T | P | (position from user input) J-Ks=0.826+/-0.035 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,12.55,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 12.55CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:50:31.21 +70:07:14.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.53 04:24:09.30 +68:13:54.7
140.67399 13.04188 galactic Cam Second-epoch detections are separated by 2.1" and 2.6 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 | SX Cam | 04:24:08.77 +68:13:18.1 (Gaia DR3) | M (local) | 2441650.00000 (local) | Gaia3var=VARIABLE SpType: M6e 1965PASP...77..392B SX Cam
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
SX Cam,2461121.7296,12.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
SX Cam 20260322.2296 12.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:09.30 +68:13:54.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 501569652378642560,2461121.7296,12.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 501569652378642560 20260322.2296 12.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:23:02.53 +73:36:54.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,12.84,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 12.84CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:31.45 +72:51:35.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.86 03:56:53.58 +67:31:31.6
139.28821 10.75294 galactic Cam Second-epoch detections are separated by 5.6" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 490316666266070784 | 03:56:48.61 +67:32:06.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 490316666266070784,2461121.7296,12.86,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 490316666266070784 20260322.2296 12.86CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:56:53.58 +67:31:31.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,12.93,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 12.93CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:16:55.61 +69:09:49.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 12.94 04:14:47.37 +68:29:33.3
139.86663 12.60197 galactic Cam Second-epoch detections are separated by 4.7" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Large-amplitude variable Gaia DR2 490781038127204608 | 04:14:42.98 +68:29:07.2 (Gaia DR3) | 2021A&A...648A..44M | | Gaia3var=NOT_AVAILABLE (the VSX policy as of May 2022 seems to be NOT to regard variables from 2021A&A...648A..44M as 'known' for the lack of classification)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Large-amplitude variable Gaia DR2 490781038127204608,2461121.7296,12.94,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Large-amplitude variable Gaia DR2 490781038127204608 20260322.2296 12.94CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:14:47.37 +68:29:33.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.01,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.01CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:29:19.14 +69:31:54.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.10,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.10CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:45:28.72 +74:16:14.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.21 04:13:48.14 +71:34:09.6
137.56062 14.71217 galactic Cam Second-epoch detections are separated by 1.6" and 2.2 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 | 04:13:48.14 +71:34:09.6 (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,2461121.7296,13.21,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.21CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:13:48.14 +71:34:09.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 496326425025087744,2461121.7296,13.09,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 496326425025087744 20260322.2296 13.09CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:47:41.12 +69:27:48.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.22,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 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-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:32:12.61 +69:46:34.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.40 03:53:26.02 +65:59:38.2
140.03489 9.36682 galactic Cam Second-epoch detections are separated by 2.5" and 1.9 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 | 03:53:26.02 +65:59:38.2 (user input) | T | P | (position from user input) J-Ks=0.893+/-0.034 (M)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.40,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.40CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:26.02 +65:59:38.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.28,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.28CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:11.95 +67:34:11.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.47 03:51:12.94 +68:31:50.8
138.21255 11.17411 galactic Cam Second-epoch detections are separated by 4.1" and 2.9 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 | 03:51:12.94 +68:31:50.8 (user input) | T | P | (position from user input) J-Ks=0.463+/-0.032 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:51:12.94 +68:31:50.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.41 06:01:11.09 +71:55:16.4
141.98900 21.92528 galactic Cam Second-epoch detections are separated by 3.2" and 3.0 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 06:01:11.09 +71:55:16.4 (user input) | T | P | (position from user input) J-Ks=0.644+/-0.032 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.41,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.41CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 06:01:11.09 +71:55:16.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.54 04:16:55.43 +72:06:22.3
137.33863 15.26116 galactic Cam Second-epoch detections are separated by 0.8" and 2.4 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 | 04:16:55.43 +72:06:22.3 (user input) | T | P | (position from user input) J-Ks=0.488+/- (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.54,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.54CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:16:55.43 +72:06:22.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.53 04:24:34.69 +69:53:54.8
139.44232 14.20227 galactic Cam Second-epoch detections are separated by 2.2" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 496933870838722048 | 04:24:27.70 +69:53:26.6 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE SpType: A 1956PMcCO..13a....B AG+69 197 J-Ks=0.524+/-0.037 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 496933870838722048,2461121.7296,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 496933870838722048 20260322.2296 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:34.69 +69:53:54.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.53 04:11:02.10 +73:32:44.3
135.95518 15.95781 galactic Cam Second-epoch detections are separated by 1.9" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:11:02.10 +73:32:44.3 (user input) | T | P | (position from user input) J-Ks=0.735+/-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,2461121.7296,13.53,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.53CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:11:02.10 +73:32:44.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.52 05:03:03.23 +74:13:01.7
137.78672 19.17983 galactic Cam Second-epoch detections are separated by 2.1" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:03.23 +74:13:01.7 (user input) | T | P | (position from user input) J-Ks=0.388+/-0.044 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:03.23 +74:13:01.7 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 493316511944154240,2461121.7296,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 493316511944154240 20260322.2296 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:53:03.79 +67:44:10.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.50 04:52:19.78 +69:40:07.4
141.20662 15.90283 galactic Cam Second-epoch detections are separated by 1.5" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 496354973668350464 | 04:52:21.27 +69:39:41.4 (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 496354973668350464,2461121.7296,13.50,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 496354973668350464 20260322.2296 13.50CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:52:19.78 +69:40:07.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.60 03:57:21.07 +71:46:52.8
136.44212 13.97595 galactic Cam Second-epoch detections are separated by 2.7" and 2.4 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 | 03:57:21.07 +71:46:52.8 (user input) | T | P | (position from user input) J-Ks=0.555+/-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,2461121.7296,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:57:21.07 +71:46:52.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.60 04:01:24.00 +70:57:54.3
137.25232 13.58663 galactic Cam Second-epoch detections are separated by 1.6" and 2.6 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:01:24.00 +70:57:54.3 (user input) | T | P | (position from user input) J-Ks=0.487+/-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,2461121.7296,13.60,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.60CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:01:24.00 +70:57:54.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.59 05:24:14.97 +70:32:24.4
141.98705 18.65326 galactic Cam Second-epoch detections are separated by 4.2" and 2.1 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:24:14.97 +70:32:24.4 (user input) | T | P | (position from user input) J-Ks=0.261+/-0.053 (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,2461121.7296,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:24:14.97 +70:32:24.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.71 04:10:46.54 +70:07:35.9
138.42821 13.51426 galactic Cam Second-epoch detections are separated by 0.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 494177906286853120 | 04:10:47.67 +70:06:56.0 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.519+/-0.036 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 494177906286853120,2461121.7296,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 494177906286853120 20260322.2296 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:10:46.54 +70:07:35.9 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.47 04:24:34.33 +67:41:11.2
141.11051 12.69850 galactic Cam Second-epoch detections are separated by 1.4" and 2.4 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 | 04:24:34.33 +67:41:11.2 (user input) | T | P | (position from user input) J-Ks=0.526+/-0.075 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.47,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.47CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:24:34.33 +67:41:11.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.65 03:58:28.05 +72:24:36.8
136.07506 14.50157 galactic Cam Second-epoch detections are separated by 4.6" and 3.1 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 | 03:58:28.05 +72:24:36.8 (user input) | T | P | (position from user input) J-Ks=0.461+/-0.076 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.65,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.65CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 03:58:28.05 +72:24:36.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.67 05:04:54.06 +70:09:41.6
141.43378 17.06897 galactic Cam Second-epoch detections are separated by 0.6" and 2.3 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:04:54.06 +70:09:41.6 (user input) | T | P | (position from user input) J-Ks=0.463+/-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,2461121.7296,13.67,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.67CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:04:54.06 +70:09:41.6 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.77 04:12:35.96 +66:58:51.0
140.80182 11.38067 galactic Cam Second-epoch detections are separated by 0.9" and 2.4 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 | 04:12:35.96 +66:58:51.0 (user input) | T | P | (position from user input) J-Ks=0.554+/- (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.77,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.77CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:12:35.96 +66:58:51.0 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.52 04:06:52.94 +65:28:29.8
141.43348 9.89274 galactic Cam Second-epoch detections are separated by 0.7" and 2.1 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 | 04:06:52.94 +65:28:29.8 (user input) | T | P | (position from user input) J-Ks=0.552+/-0.035 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.52,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.52CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:06:52.94 +65:28:29.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 J042521.6+685943,2461121.7296,13.71,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
WISE J042521.6+685943 20260322.2296 13.71CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:25:21.61 +68:59:43.3 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.79 05:03:14.16 +72:34:09.2
139.25042 18.28852 galactic Cam Second-epoch detections are separated by 0.6" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 05:03:14.16 +72:34:09.2 (user input) | T | P | (position from user input) J-Ks=0.493+/-0.043 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.79,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.79CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:03:14.16 +72:34:09.2 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.59 04:20:12.28 +67:58:51.8
140.60096 12.60207 galactic Cam Second-epoch detections are separated by 1.9" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:20:12.28 +67:58:51.8 (user input) | T | P | (position from user input) J-Ks=0.806+/-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,2461121.7296,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:20:12.28 +67:58:51.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.59 05:16:13.51 +71:25:49.4
140.82880 18.53330 galactic Cam Second-epoch detections are separated by 2.6" and 2.5 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | Gaia DR3 498063893914090752 | 05:16:12.40 +71:26:30.1 (Gaia DR3) | T | P | Gaia3var=NOT_AVAILABLE J-Ks=0.641+/-0.039 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
Gaia DR3 498063893914090752,2461121.7296,13.59,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 498063893914090752 20260322.2296 13.59CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:16:13.51 +71:25:49.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.80 04:56:17.89 +70:32:23.4
140.67947 16.68818 galactic Cam Second-epoch detections are separated by 1.3" and 2.2 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:56:17.89 +70:32:23.4 (user input) | T | P | (position from user input) J-Ks=0.429+/-0.046 (G)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.80,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.80CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:56:17.89 +70:32:23.4 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Mean magnitude and position on the discovery images:
2026 03 22.2296 2461121.7296 13.78 04:31:50.03 +66:09:34.8
142.75682 12.19605 galactic Cam Second-epoch detections are separated by 2.8" and 2.7 pix
The object was not found in VSX
The object was not found in ASASSN-V
The object was not found in astcheck.
online_id | target | 04:31:50.03 +66:09:34.8 (user input) | T | P | (position from user input) J-Ks=0.526+/-0.037 (K)
Check this position in TNS.Search this object in SIMBAD.Search this object in VizieR catalogs.WISE atlasAladin LiteSNAD ZTF viewer
Online MPChecker may fail to identify bright comets! Please manually check the Seiichi Yoshida's and Gideon van Buitenen's pages.
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#SOFTWARE=VaST 1.0rc89 transient pipeline
#DELIM=,
#DATE=JD
#NAME,DATE,MAG,MERR,FILT,TRANS,MTYPE,CNAME,CMAG,KNAME,KMAG,AMASS,GROUP,CHART,NOTES
target,2461121.7296,13.78,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
target 20260322.2296 13.78CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 04:31:50.03 +66:09:34.8 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
Don't forget to copy the leading white spaces and change the observatory code!
The code 'C32' is 'Ka-Dar Observatory, TAU Station, Nizhny Arkhyz', the code '500' is the geocenter.
Make sure there are no trailing white spaces after the observatory code.
The string should be exactly 80 characters long to conform to the MPC format.
Mean position:
You may copy/paste the above measurements to the following online services: MPChecker (in case the button does not work) NEOCMTChecker (NEO's and comets) sat_id2 (artificial satellites; needs at least two observations to work) fitsblink_satellites (art. sat.; you'll need to save the astrometry as a text file and upload it)
Here is a stub line for reporting a new transient to the TOCP.
Don't forget to set the constellation name and the number of days since the last non-detection!
Don't forget to change the observer code for the AAVSO and VSNET format data!
**** AAVSO file format ****
#TYPE=EXTENDED
#OBSCODE=SKA
#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 485261519820258560,2461121.7296,11.26,0.05,CV,NO,STD,ENSEMBLE,na,na,na,na,1,na,NMW-TexasTech Camera-2 135mm f/2.2 telephoto lens + QHY600M CMOS
**** VSNET file format ****
# Here are some valid formatiing examples:
#CETFZ 20230815.9829 <13.5CV NMW
#CETFZ 20230818.9746 12.5CV NMW
#CETFZ 20230819.9732 12.6CV NMW
#TCPJ17453768-1756253 20230831.7290 12.7CV NMW
Gaia DR3 485261519820258560 20260322.2296 11.26CV NMW
The AAVSO data should be submitted to https://www.aavso.org/webobs
The VSNET data, depending on how interesting the target is, should be e-mailed to
vsnet-alert@ooruri.kusastro.kyoto-u.ac.jp
vsnet-outburst-wanted@ooruri.kusastro.kyoto-u.ac.jp
vsnet-obs@ooruri.kusastro.kyoto-u.ac.jp
# Time-series data may be sent to vsnet-campaign-report@ooruri.kusastro.kyoto-u.ac.jp
# Set SExtractor parameters file
cp default.sex.telephoto_lens_onlybrightstars_v1 default.sex
# Plate-solve the FITS images and produce the finder charts
export TELESCOP=''
for i in /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits ;do util/wcs_image_calibration.sh $i && util/make_finding_chart_script.sh wcs_`basename $i` 05:59:26.94 +70:48:57.5 ;done
# Combine the finder charts into one image (note the '*' symbols meaning the command will work only if you have a single transient in that field)
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v1.png
montage resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix_nofov.png -tile 2x1 -geometry +0+0 finder_chart_v2.png
# Create GIF animation
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20_00sec_-15_00C_LIGHT_0095_fits__*pix.png animation_v1.gif
convert -delay 50 -loop 0 resample_wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20_00sec_-14_90C_LIGHT_0399_fits__*pix.png resample_wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20_00sec_-14_90C_LIGHT_0094_fits__*pix.png animation_v2.gif
## VaST run with SExtractor config file default.sex.telephoto_lens_onlybrightstars_v1 ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
First image: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Last image: 2461121.72981475 22.03.2026 05:30:45.994 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 8
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: 7 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): 14414
Objects passed selection criteria: 14401
Measurements per detected object (mean, median, min, max): 3.6 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.6 4.0 2 4
Average stars detected per image: 13329.2
Average stars matched: 12823.2 (96.2038 %)
Memory usage VmPeak: 119304 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 02:18:41 CDT 2026
Host name: tau
############################################################
## VaST run with SExtractor config file default.sex.telephoto_lens_vSTL ##
Images processed 4
Images used for photometry 4
Ref. image: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
First image: 2461032.82849338 23.12.2025 07:52:51.828 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Last image: 2461121.72981475 22.03.2026 05:30:45.994 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
JD time system (TT/UTC/UNKNOWN): UTC
Transient candidates found: 482
FILTER key from ref. img. header: CV
Magnitude scale: instrumental
Estimated ref. image limiting mag.: -7.29
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: 38 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): 98435
Objects passed selection criteria: 98204
Measurements per detected object (mean, median, min, max): 3.5 4.0 2 4
Measurements per selected object (mean, median, min, max): 3.5 4.0 2 4
Average stars detected per image: 89088.2
Average stars matched: 85530.5 (96.0065 %)
Memory usage VmPeak: 1929064 kB
Software: VaST 1.0rc89 compiled with gcc (Gentoo 15.2.1_p20251122 p4) 15.2.1 20251122
VaST compiled on Sat Mar 21 15:05:04 CDT 2026
VaST build number 1.0rc88-354-ge3e751fc
OpenMP enabled: Yes
SExtractor version 2.19.5 (2026-03-21)
GNU bash, version 5.3.9(1)-release (x86_64-pc-linux-gnu)
Processing completed on Sun Mar 22 02:20:12 CDT 2026
Host name: tau
############################################################
Updating neverexclude_list.txt
'/var/www/nmw_calibration/neverexclude_list.txt' -> './neverexclude_list.txt'
Choosing bad regions list
'/var/www/nmw_calibration/TTUQ2b1x1/TTUQ2_bad_region.lst' -> 'bad_region.lst'
wait
*------ default.sex.telephoto_lens_onlybrightstars_v1 ------*
'default.sex.telephoto_lens_onlybrightstars_v1' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_onlybrightstars_v1
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
SExtractor catalog cache: saved Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat to cache
SExtractor catalog cache: saved Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_onlybrightstars_v1
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
Checking WCS cache directory local_wcs_cache
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
The reference JD(UT) for computing planet and comet positions: 2461121.72929418
Re-using ../asassn_transients_list.txt
'../asassn_transients_list.txt' -> 'asassn_transients_list.txt'
Plate-solving the images
'tocp_transients_list.txt' -> '../tocp_transients_list.txt'
wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits exists and is non-empty
Saving wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits to local_wcs_cache/
'wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> 'local_wcs_cache/wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits'
wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits exists and is non-empty
Saving wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits to local_wcs_cache/
'wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> 'local_wcs_cache/wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits'
wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits'
wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits exists and is non-empty
Saving wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits to local_wcs_cache/
'wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits' -> 'local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.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 04:47:15.618 +69:59:24.55
Angular distance between the image centers 0.05 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 04:47:14.967 +69:59:38.23
Angular distance between the image centers 0.05 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 04:47:15.618 +69:59:24.55
Second-epoch second image center 04:47:14.967 +69:59:38.23
Angular distance between the image centers 0.00391 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits &> /tmp/tmp.QRZIXgKfFx
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits &> /tmp/tmp.cnYRHAUQHq
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits &> /tmp/tmp.jjVdBVzBsj
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits &> /tmp/tmp.Zjxp3z5gPk
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Found non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
The reference image (wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits) and catalog (wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat) found
'wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 58 out of 16183 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 22.881698
a=0.000000 b=1.000000 c=22.881698
From vast_summary.log: estimated ref. image limiting mag.: -7.62
Updating vast_summary.log: Estimated ref. image limiting mag.: 15.26
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 15.26
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 7 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
2.1 pix Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
2.1 pix Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
2.5 pix fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
2.5 pix fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
Limiting magnitude estimates:
15.3 mag. Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
15.2 mag. Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
15.0 mag. fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
15.0 mag. fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
All-image limiting magnitude estimate: 15.0 (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 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.QRZIXgKfFx (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> 'wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1300, passed=16183
Got 16183 stars (including 14865 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
util/solve_plate_with_UCAC5 got 16183 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.3'
Seting catalog search parameters based on the expected field of view 931.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012935 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010348 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 292 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.79"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.09"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 360 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.02"
Estimated accuracy of the plate solution: 5.56"
Excluding outliers - 323 stars left (next iteration limit 245)
The image catalog is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits -region wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.cnYRHAUQHq (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> 'wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=1282, passed=16167
Got 16167 stars (including 14867 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat
util/solve_plate_with_UCAC5 got 16167 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.38"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.35"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 968 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.35"
Estimated accuracy of the plate solution: 0.35"
Excluding outliers - 967 stars left (next iteration limit 1063)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits -region wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.jjVdBVzBsj (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=944, passed=15286
Got 15286 stars (including 14329 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits.cat
util/solve_plate_with_UCAC5 got 15286 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.51"
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: 0.51"
Estimated accuracy of the plate solution: 0.48"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits -region wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.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.Zjxp3z5gPk (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=0, blended=976, passed=15254
Got 15254 stars (including 14268 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits.cat
util/solve_plate_with_UCAC5 got 15254 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 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: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 970 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.50"
Estimated accuracy of the plate solution: 0.47"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits -region wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits'
Saving fully-calibrated image wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits'
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits'
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
'wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits' -> '/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits'
Preparing the HTML report for the field Cam-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
Adding exclusion_list_gaiadr2.txt__out20882.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21355.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21370.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21393.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21471.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21479.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out21495.dat to exclusion_list_gaiadr2.txt
make_report_in_HTML.sh Phase 1 (network queries): 1s
Pre-generating preview images in parallel...
Done pre-generating preview images.
Pre-generating finding charts in parallel...
Done pre-generating finding charts.
make_report_in_HTML.sh Pre-generation: 0s
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Considering the candidate 20882_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 20882_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 05:35:24.73 +72:03:08.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 5.206 498507134538498048 083.85773222768 +72.05237071573 12.3021 11.8045 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#5.206#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21355_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 21355_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 04:37:53.96 +71:27:17.0 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.06, MAG_FAINT_SEARCH_LIMIT=13.04)GAIADR2_OUTPUT=# 0.767 500535802212355456 069.47518647410 +71.45454129490 11.9885 11.5352 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.767#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21370_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 21370_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 05:20:10.33 +71:33:54.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.04, MAG_FAINT_SEARCH_LIMIT=13.02)GAIADR2_OUTPUT=# 0.745 498147899176343936 080.04274431906 +71.56495450163 11.8098 11.0125 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.745#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21393_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 21393_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 04:50:20.56 +68:09:06.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.10, MAG_FAINT_SEARCH_LIMIT=13.08)GAIADR2_OUTPUT=# 0.357 495967984234117504 072.58584113756 +68.15164736946 12.0959 11.3506 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.357#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21471_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 21471_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 05:04:24.06 +69:47:50.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.27, MAG_FAINT_SEARCH_LIMIT=13.25)GAIADR2_OUTPUT=# 0.033 496231587848912128 076.10027246800 +69.79728243252 12.0807 11.4351 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.033#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21479_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 21479_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 04:44:31.29 +72:48:36.8 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.37, MAG_FAINT_SEARCH_LIMIT=13.35)GAIADR2_OUTPUT=# 0.946 500908669794258688 071.13116150341 +72.81009943899 10.8924 9.5397 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.946#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 21495_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 21495_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 05:08:42.10 +70:40:44.1 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.34, MAG_FAINT_SEARCH_LIMIT=13.32)GAIADR2_OUTPUT=# 0.227 497961123936904320 077.17528803194 +70.67887022278 12.3427 11.9350 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.227#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
make_report_in_HTML.sh Phase 2 (HTML assembly): 0s
make_report_in_HTML.sh TOTAL: 1s
Prepared the HTML report for the field Cam-06-Q2b1x1 with default.sex.telephoto_lens_onlybrightstars_v1
*------ done with default.sex.telephoto_lens_onlybrightstars_v1 ------*
#### The local exclusion list is exclusion_list_local.txt ####
wait
*------ default.sex.telephoto_lens_vSTL ------*
'default.sex.telephoto_lens_vSTL' -> 'default.sex'
Starting VaST with default.sex.telephoto_lens_vSTL
./vast --norotation --noflagimage --starmatchraius 4 --matchstarnumber 500 --selectbestaperture --sysrem 0 --type 4 --maxsextractorflag 99 --UTC --nofind --nojdkeyword /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
SExtractor catalog cache: saved Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat to cache
SExtractor catalog cache: saved Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat to cache
VaST run complete with default.sex.telephoto_lens_vSTL
The four input images were /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
Checking WCS cache directory local_wcs_cache
Found WCS cache directory local_wcs_cache
Creating symlink local_wcs_cache/wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Creating symlink local_wcs_cache/wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
Creating symlink local_wcs_cache/wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
Creating symlink local_wcs_cache/exclusion_list.txt
Checking WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Found WCS cache directory /mnt/usb/NMW_NG/solved_reference_images
Checking WCS cache directory /home/NMW_web_upload/solved_reference_images
Checking WCS cache directory /dataX/kirx/NMW_NG_rt3_autumn2019/solved_reference_images
Plate-solving the images
wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits exists and is non-empty
wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits exists and is non-empty
wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits exists and is non-empty
wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.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 04:47:15.618 +69:59:24.55
Angular distance between the image centers 0.05 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 04:47:14.967 +69:59:38.23
Angular distance between the image centers 0.05 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 04:47:15.618 +69:59:24.55
Second-epoch second image center 04:47:14.967 +69:59:38.23
Angular distance between the image centers 0.00391 deg.
###################################
Running solve_plate_with_UCAC5...
Preparing for ar aprallel run
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits &> /tmp/tmp.B8tJGddHlE
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits &> /tmp/tmp.8FFDaaDBRZ
Parallel run for /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits &> /tmp/tmp.dOJQG3f03Y
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
Running util/solve_plate_with_UCAC5 --no_photometric_catalog --iterations 2 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits &> /tmp/tmp.iaEPm8yylF
Parallel run for /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
Calibrating the magnitude scale
Found non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
____ Start of magnitude calibration ____
PHOTOMETRIC_CALIBRATION=TYCHO2_V
Calibrating the magnitude scale with Tycho-2 stars
util/transients/transient_factory_test31.sh is checking for the presence of non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Tycho-2 catalog is found at lib/catalogs/tycho2
Tycho-2 catalog and the derived bright star exclusion list are ready
Checking for the presence of non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
Found non-empty wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits and wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
The reference image (wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits) and catalog (wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat) found
'wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat' -> 'wcsmag.cat'
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.00
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.01
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.02
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.03
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.04
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.05
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.06
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.07
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.08
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.09
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.10
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.11
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.12
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.13
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.14
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.15
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.16
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.17
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.18
Reading Tycho2 catalog file lib/catalogs/tycho2/tyc2.dat.19
Relation between the catalog and instrumental magnitudes is written to calib.txt
Matched with Tycho-2 85 out of 113524 detected stars.
The calibration function type and coefficients are written to calib.txt_param
util/calibrate_magnitude_scale 0.000000 1.000000 21.485424
a=0.000000 b=1.000000 c=21.485424
From vast_summary.log: estimated ref. image limiting mag.: -7.29
Updating vast_summary.log: Estimated ref. image limiting mag.: 14.20
Updated vast_limiting_magnitude.log with calibrated magnitudes
Working...
Please, PLEASE, be patient!!!
All lightcurves processed! =)
Estimated ref. image limiting mag.: 14.20
Magnitude calibration plot:
____ End of magnitude calibration ____
Applying consolidated magnitude filters...
Preparing the exclusion lists for this field
Done with filtering
Found 347 candidate transients before the final filtering. (Hard limit: 3000)
Median FWHM seeing for isolated stars:
1.9 pix Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
1.9 pix Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
2.4 pix fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
2.4 pix fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
Limiting magnitude estimates:
14.2 mag. Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
14.2 mag. Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
13.9 mag. fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
13.9 mag. fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
All-image limiting magnitude estimate: 13.9 (SNR ) 13.2 (80% of stars) with default.sex.telephoto_lens_vSTL
The first estimate is the magnitude of a star detected with a signal-to-noise ratio of following Karpov (2025, Acta Polytechnica, 65, 50).
This value should be representative of the faintest stars clearly visible in the image.
The brighter of the limiting magnitude estimates for the two second-epoch images is reported here.
The second estimate is the 80th percentile of the magnitude distribution of stars detected on all four images.
This value is representative of the faintest object that may enter the candidate transients list.
The hard cut-off for the candidate transients is 15.0 mag.
Waiting for UCAC5 plate solver
wait
############ /tmp/tmp.B8tJGddHlE (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits 570.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits' -> 'wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=31, blended=9713, passed=113493
Got 113493 stars (including 103609 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat
util/solve_plate_with_UCAC5 got 113493 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 931.3'
Seting catalog search parameters based on the expected field of view 931.3 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.012935 (46.6 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010348 (37.3 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 303 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.36"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 6.47"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 368 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 6.45"
Estimated accuracy of the plate solution: 5.59"
Excluding outliers - 329 stars left (next iteration limit 266)
The image catalog is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits -region wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.8FFDaaDBRZ (6) ############
Parsing command line arguments...
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits is already a symlink and we do not allow symlinks on symlinks
The guess is based on the existing WCS header.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits 573.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WARNING from replace_file_with_symlink_if_filename_contains_white_spaces() the input file /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits is already a symlink and we do not allow symlinks on symlinks
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
verification OK: /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
It's a known telescope with plate solutions that are supposed to be good.
The input image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits has a WCS header - will blindly trust it is good...
'/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits' -> 'wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits'
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS_IMAGE_NAME=wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS-calibrated image found: wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Checking if the catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits alredy exist and is non-empty...
Catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat corresponding to the image wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
WCS catalog name: wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=9545, passed=112768
Got 112768 stars (including 103038 good ones) from the SExtractor catalog wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat
util/solve_plate_with_UCAC5 got 112768 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 941.6'
Seting catalog search parameters based on the expected field of view 941.6 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013078 (47.1 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010462 (37.7 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.37"
ITERATION 02 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 969 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.37"
Estimated accuracy of the plate solution: 0.36"
Excluding outliers - 968 stars left (next iteration limit 1064)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/reference_imgs/Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits -region wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
############ /tmp/tmp.dOJQG3f03Y (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=17, blended=7255, passed=87585
Got 87585 stars (including 80249 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits.cat
util/solve_plate_with_UCAC5 got 87585 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 965 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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 966 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Estimated accuracy of the plate solution: 0.49"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 964 stars left (next iteration limit 1060)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits -region wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.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.iaEPm8yylF (6) ############
Parsing command line arguments...
The minor axis of the CCD chip should be 24.0 mm based on the derived pixel size of 3.8 um
Internal estimated FoV 605.3'
The guess is based on the FOCALLEN keyword.
Trying to blindly solve the plate (local solve-field or remote server)...
/data_ssd/NMW-TexasTech/workdir/vast_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/util/wcs_image_calibration.sh /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits 605.0
Entering WCS image calibration mode.
ORIGINAL_FITSFILE=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
FITSFILE before on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
verification OK: /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
It's not one of the telescopes that are know to produce images with good WCS solutions - will try to re-solve!
FITSFILE after on_the_fly=/data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
WCS_IMAGE_NAME=wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
WCS-calibrated image found: wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
Checking if the catalog wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits alredy exist and is non-empty...
Catalog wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits.cat corresponding to the image wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits found.
The catalog is in the new format, as expected.
The plate-solved (WCS-calibrated) image is saved to wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
util/solve_plate_with_UCAC5 is preparing to read a catalog corresponding to the image /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
WCS catalog name: wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits.cat
SExtractor catalog parsing summary: zero_flux=0, no_flux_err=0, no_mag=0, no_mag_err=0, low_SNR=18, blended=7504, passed=88595
Got 88595 stars (including 80999 good ones) from the SExtractor catalog wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits.cat
util/solve_plate_with_UCAC5 got 88595 stars from the SExtractor catalog
Updated FoV from the plate-solved image: 937.8'
Seting catalog search parameters based on the expected field of view 937.8 arcmin
UCAC5 catalog search parameters:
catalog_search_parameters->search_radius_deg= 0.013025 (46.9 arcsec)
catalog_search_parameters->brightest_mag= 1.00
catalog_search_parameters->faintest_mag= 13.50
catalog_search_parameters->search_radius_second_step_deg 0.010420 (37.5 arcsec)
ITERATION 01 -- talking to VizieR, this might be slow!
UCAC5 search strategy: trying local copy first
Found a local copy of UCAC5
Reading UCAC5 zone files...
Done reading UCAC5 zone files...
Matched 967 stars with the local copy of UCAC5.
The local UCAC5 search seems to be a success
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.50"
Removing outliers...
Correcting the measured astrometric positions...
Estimated accuracy of the plate solution: 0.49"
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: 0.49"
Estimated accuracy of the plate solution: 0.49"
Excluding outliers - 966 stars left (next iteration limit 1062)
Stop iterations.
The field is successfully solved and matched with the astrometric catalog! :)
The image catalog is written to wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits.cat.ucac5
The DS9 region file with the matched stars is written to wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits.cat.ds9.reg
You may view it with the command:
ds9 /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits -region wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits.cat.ds9.reg
The astrometric residuals vector field is written to wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits.cat.astrometric_residuals
Option '-n' not using photometric catalogs, just stick with astrometry
opt '-i': 2 is the maximum number of iterations
Copying WCS-calibrated images back to input directory
Saving fully-calibrated image wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/wcs_Cam-06-Q2b1x1_2025-12-23_01-52-51_20.00sec_-14.90C_LIGHT_0399.fits
Saving fully-calibrated image wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/wcs_Cam-06-Q2b1x1_2025-12-23_01-53-30_20.00sec_-15.00C_LIGHT_0400.fits
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-01_20.00sec_-14.90C_LIGHT_0094.fits
Saving fully-calibrated image wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
INFO: FPACK_FULLY_CALIBRATED_IMAGE=no (not compressing the image)
The destination file is already there - not rewriting /data_ssd/NMW-TexasTech/workdir//img_2026-03-22_CI_Cam-06-Q2b1x1_013113_TTUQ2b1x1_2947_NypQwLqx/wcs_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095.fits
Preparing the HTML report for the field Cam-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
Adding exclusion_list_gaiadr2.txt__out131948.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132014.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132023.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out132027.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133846.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out133961.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135477.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135542.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out135743.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out136044.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_gaiadr2.txt__out136217.dat to exclusion_list_gaiadr2.txt
Adding exclusion_list_local.txt__out131931.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131942.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131947.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131949.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131957.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131959.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131962.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131974.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131983.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131984.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131985.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131986.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131989.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131990.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131995.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131996.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out131998.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132001.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132004.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132006.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132007.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132017.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132025.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out132703.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133212.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133267.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133529.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133835.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out133969.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134086.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134138.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134179.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134280.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134399.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134515.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134641.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134725.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out134841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135108.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135146.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135155.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135317.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135597.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135665.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135681.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135719.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135747.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135751.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135756.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135781.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135841.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135872.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135895.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135911.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135948.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out135960.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136003.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136021.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136064.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136087.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136112.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136145.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136192.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136223.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136269.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136282.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out136295.dat to exclusion_list_local.txt
Adding exclusion_list_local.txt__out27970.dat to exclusion_list_local.txt
make_report_in_HTML.sh Phase 1 (network queries): 103s
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: 48s
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Considering the candidate 131931_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 131931_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 131942_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 131942_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 131947_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 131947_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 131948_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 131948_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 04:56:22.16 +72:43:27.3 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.56, MAG_FAINT_SEARCH_LIMIT=14.54)GAIADR2_OUTPUT=# 1.077 500719626811529216 074.09326796345 +72.72413824631 14.5230 13.6680 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.077#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 131949_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 131949_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 131957_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 131957_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 131959_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 131959_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 131962_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 131962_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 131974_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 131974_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 131981_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 131981_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 131983_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 131983_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 131984_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 131984_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 131985_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 131985_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 131986_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 131986_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 131989_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 131989_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 131990_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 131990_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 131995_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 131995_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 131996_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 131996_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 131998_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 131998_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 132001_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 132001_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 132004_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 132004_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 132006_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 132006_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 132007_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 132007_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 132008_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132008_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 132014_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132014_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 03:48:56.89 +65:32:20.4 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.26, MAG_FAINT_SEARCH_LIMIT=13.24)GAIADR2_OUTPUT=# 0.523 488357027307740544 057.23722571476 +65.53912352695 13.0320 11.8593 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.523#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132017_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 132017_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 132023_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132023_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 03:53:20.42 +67:29:25.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=11.44, MAG_FAINT_SEARCH_LIMIT=12.42)GAIADR2_OUTPUT=# 1.081 493292494487455488 058.33531621740 +67.49013004764 12.0913 10.9203 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.081#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132024_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132024_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (10.4") between the two second-epoch detections
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Considering the candidate 132025_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 132025_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 132026_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132026_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 132027_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132027_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 03:51:38.72 +65:42:38.5 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN= 9.55, MAG_FAINT_SEARCH_LIMIT=10.53)GAIADR2_OUTPUT=# 1.153 489857414003291648 057.91074760453 +65.71048326605 10.2351 9.1109 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.153#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 132489_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132489_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 132521_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132521_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 132564_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132564_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 132618_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132618_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 132659_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132659_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 132665_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132665_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 132680_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132680_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 132703_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 132703_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 132720_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132720_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 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 132733_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132733_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 132753_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132753_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 132761_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132761_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 132785_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132785_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 132816_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132816_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 132830_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132830_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 132848_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132848_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 132873_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132873_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 132878_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132878_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 132893_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132893_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 132894_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132894_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 132910_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132910_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 132930_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132930_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 04:13:40.79 +72:09:24.0 in the exclusion list exclusion_list_bsc.txt ****
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Considering the candidate 132946_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132946_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 132961_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 132961_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 133015_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133015_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 133017_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133017_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 133036_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133036_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 133047_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133047_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 133055_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133055_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133062_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133062_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 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 133064_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133064_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 133065_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133065_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 133106_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133106_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 133154_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133154_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 133200_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133200_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 133204_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133204_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 133212_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 133212_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 133213_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133213_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 133237_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133237_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 133251_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133251_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 133267_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 133267_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 133273_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133273_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 133305_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133305_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 133342_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133342_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 133344_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133344_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 133345_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133345_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 133372_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133372_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 133378_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133378_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 133412_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133412_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 133441_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133441_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 133448_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133448_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 133451_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133451_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 133464_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133464_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 133481_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133481_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 133515_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133515_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 133518_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133518_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 133529_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 133529_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 133543_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133543_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 133556_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133556_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 133563_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133563_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 133608_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133608_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 133611_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133611_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 133618_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133618_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 133622_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133622_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 133690_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133690_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 133695_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133695_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 133702_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133702_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 133712_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133712_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 133759_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133759_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 133770_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133770_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 133778_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133778_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 133799_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133799_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 133802_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133802_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 133808_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133808_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 133835_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 133835_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 133837_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133837_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 133846_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133846_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 03:37:38.73 +69:10:28.2 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.43, MAG_FAINT_SEARCH_LIMIT=13.41)GAIADR2_OUTPUT=# 0.814 494403585346278912 054.41074096462 +69.17451905166 13.1554 12.1513 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.814#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133884_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133884_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 133904_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133904_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 133911_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133911_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 133914_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133914_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 133919_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133919_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 133933_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133933_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 133942_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133942_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 133947_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133947_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 133961_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133961_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 04:17:16.33 +66:57:56.9 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=12.45, MAG_FAINT_SEARCH_LIMIT=13.43)GAIADR2_OUTPUT=# 1.733 489701042833419648 064.31682306768 +66.96573963736 12.3157 10.3326 VARIABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.733#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 133969_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 133969_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 133987_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133987_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 133992_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 133992_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 134024_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134024_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 134031_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134031_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 134048_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134048_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134056_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134056_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134077_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134077_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 134083_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134083_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 134086_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 134086_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 134099_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134099_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 134103_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134103_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 134120_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134120_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 134126_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134126_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 134134_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134134_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 134138_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 134138_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134142_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134142_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 134149_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134149_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 134152_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134152_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 134157_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134157_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 134170_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134170_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 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 134176_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134176_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 134179_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 134179_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 134181_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134181_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 134224_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134224_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 134236_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134236_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 134238_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134238_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 134252_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134252_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 134255_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134255_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 134265_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134265_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 134272_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134272_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 134280_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 134280_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 134307_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134307_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 134316_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134316_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 134321_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134321_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 134323_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134323_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 134324_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134324_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 134329_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134329_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 134375_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134375_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 134383_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134383_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 134384_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134384_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 134393_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134393_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 134399_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 134399_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 134405_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134405_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 134410_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134410_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 134411_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134411_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 134436_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134436_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 134462_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134462_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 134469_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134469_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 134515_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 134515_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134531_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134531_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 134548_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134548_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 134566_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134566_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 134573_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134573_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 134585_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134585_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134589_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134589_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134590_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134590_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134628_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134628_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134631_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134631_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134641_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 134641_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134654_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134654_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134657_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134657_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134665_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134665_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134668_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134668_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134697_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134697_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134725_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 134725_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134746_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134746_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.8") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134759_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134759_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134762_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134762_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134773_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134773_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134777_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134777_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134785_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134785_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134802_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134802_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134811_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134811_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134813_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134813_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134818_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134818_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134841_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 134841_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 134846_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134846_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 134886_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134886_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 134892_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134892_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 134894_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134894_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 134917_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134917_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 134919_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134919_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 134921_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134921_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 134930_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134930_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 134940_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134940_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 134965_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134965_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 134978_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134978_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 134990_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134990_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 134991_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 134991_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 135006_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135006_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 135008_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135008_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.2") between the two second-epoch detections
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Considering the candidate 135019_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135019_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 135032_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135032_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 135041_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135041_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 135050_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135050_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 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 135056_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135056_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 135059_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135059_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 135061_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135061_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 135063_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135063_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 135068_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135068_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 135071_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135071_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 135108_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135108_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 135115_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135115_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 135132_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135132_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 135146_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135146_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 135149_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135149_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 135155_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135155_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 135178_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135178_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 135183_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135183_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 135189_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135189_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 135214_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135214_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 135223_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135223_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 135247_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135247_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 135251_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135251_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 135254_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135254_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 135271_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135271_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
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Considering the candidate 135272_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135272_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 135284_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135284_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 135287_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135287_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 135303_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135303_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 135314_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135314_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 135317_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135317_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 135338_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135338_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (11.0") between the two second-epoch detections
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Considering the candidate 135352_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135352_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 135372_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135372_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (11.3") between the two second-epoch detections
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Considering the candidate 135420_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135420_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 135469_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135469_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 135477_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135477_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 03:53:31.46 +65:45:06.7 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.47, MAG_FAINT_SEARCH_LIMIT=14.45)GAIADR2_OUTPUT=# 0.650 489852466201250560 058.38149515136 +65.75179787426 14.3592 13.3206 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.650#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135486_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135486_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
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Considering the candidate 135495_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135495_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 135498_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135498_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 135502_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135502_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 135509_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135509_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 135515_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135515_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 135524_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135524_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 135526_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135526_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 135536_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135536_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
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Considering the candidate 135542_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135542_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 04:01:41.25 +70:13:00.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 2.541 494224193151834496 060.42391281977 +70.21668301171 14.4545 13.5481 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#2.541#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
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Considering the candidate 135554_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135554_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 135560_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135560_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
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Considering the candidate 135566_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135566_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.8") between the two second-epoch detections
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Considering the candidate 135596_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135596_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
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Considering the candidate 135597_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135597_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 135631_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135631_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 135638_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135638_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 135641_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135641_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 135648_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135648_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
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Considering the candidate 135655_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135655_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 135665_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135665_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 135681_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135681_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135694_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135694_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
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Considering the candidate 135711_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135711_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 135713_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135713_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
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Considering the candidate 135719_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135719_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135728_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135728_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.1") between the two second-epoch detections
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Considering the candidate 135731_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135731_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 135743_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135743_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 03:41:55.76 +68:36:20.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.66, MAG_FAINT_SEARCH_LIMIT=14.64)GAIADR2_OUTPUT=# 1.442 494314971581606912 055.48320891483 +68.60596376474 14.5188 13.8032 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.442#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135747_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135747_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135751_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135751_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135756_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135756_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135767_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135767_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 135769_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135769_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
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Considering the candidate 135781_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135781_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
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Considering the candidate 135791_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135791_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.6") between the two second-epoch detections
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Considering the candidate 135806_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135806_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
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Considering the candidate 135808_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135808_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 135812_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135812_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.0") between the two second-epoch detections
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Considering the candidate 135815_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135815_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.4") between the two second-epoch detections
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Considering the candidate 135823_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135823_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 135825_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135825_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
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Considering the candidate 135840_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135840_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
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Considering the candidate 135841_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135841_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135843_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135843_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
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Considering the candidate 135848_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135848_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.5") between the two second-epoch detections
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Considering the candidate 135858_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135858_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.3") between the two second-epoch detections
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Considering the candidate 135859_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135859_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135869_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135869_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135872_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135872_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135877_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135877_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (16.3") between the two second-epoch detections
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Considering the candidate 135892_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135892_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
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Considering the candidate 135895_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135895_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135909_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135909_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.8") between the two second-epoch detections
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Considering the candidate 135911_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135911_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135914_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135914_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (10.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135938_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135938_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135948_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135948_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135960_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 135960_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135966_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135966_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 135967_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135967_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (16.4") between the two second-epoch detections
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Considering the candidate 135975_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 135975_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136003_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 136003_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136011_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136011_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 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 136021_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 136021_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136040_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136040_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136044_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136044_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 04:17:29.14 +67:32:26.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.53, MAG_FAINT_SEARCH_LIMIT=14.51)GAIADR2_OUTPUT=# 0.933 490483792033360640 064.37209486686 +67.54071905091 14.4360 13.4740 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#0.933#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136048_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136048_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136052_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136052_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136053_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136053_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136057_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136057_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.3") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136064_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 136064_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136077_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136077_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136087_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 136087_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136089_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136089_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136103_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136103_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (12.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136105_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136105_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136112_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 136112_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136119_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136119_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136128_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136128_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136135_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136135_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136137_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136137_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.9") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136145_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 136145_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136160_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136160_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136178_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136178_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136192_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 136192_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136207_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136207_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136217_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136217_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
**** FOUND 04:35:07.83 +67:31:59.6 in Gaia DR2 single (GAIA_DR2_CLIENT=#vizquery#, MAG_MEAN=13.63, MAG_FAINT_SEARCH_LIMIT=14.61)GAIADR2_OUTPUT=# 1.703 495515157242312576 068.78332419988 +67.53361246442 14.5697 13.5903 NOT_AVAILABLE#N_GAIA_STARS_WITIN_BLEND_SEARCH_RADIUS=#1#DISTANCE_ARCSEC=#1.703#MAX_ANGULAR_DISTANCE_BETWEEN_MEASURED_POSITION_AND_CATALOG_MATCH_ARCSEC=#5.8#
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136223_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 136223_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136247_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136247_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.1") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136252_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136252_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (11.2") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136269_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 136269_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136276_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136276_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (13.4") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136282_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 136282_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136295_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 136295_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 136379_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 136379_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 60390_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 60390_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.6") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 25035_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 25035_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (12.5") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 63207_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 63207_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (14.7") between the two second-epoch detections
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 27970_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
Preparing report for the candidate 27970_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
xxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxxx
Considering the candidate 16918_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095
The candidate 16918_fd_Cam-06-Q2b1x1_2026-03-22_00-30-45_20.00sec_-15.00C_LIGHT_0095 did not pass the final checks
Rejecting candidate due to large distance (15.0") between the two second-epoch detections
make_report_in_HTML.sh Phase 2 (HTML assembly): 13s
make_report_in_HTML.sh TOTAL: 164s
Prepared the HTML report for the field Cam-06-Q2b1x1 with default.sex.telephoto_lens_vSTL
*------ done with default.sex.telephoto_lens_vSTL ------*
#### The local exclusion list is exclusion_list_local.txt ####
04:49:03.90 +69:07:44.0
06:20:35.20 +72:57:44.3
04:28:03.62 +70:46:00.9
05:15:41.24 +72:19:02.5
04:24:09.95 +70:35:42.9
04:19:02.37 +69:20:47.4
04:20:24.98 +74:02:54.5
04:12:12.07 +72:09:08.5
04:15:21.53 +66:29:41.3
03:50:31.20 +66:54:01.6
04:15:29.39 +66:00:07.2
03:41:01.16 +69:27:18.3
04:01:13.81 +67:58:11.5
04:11:33.42 +65:34:22.7
03:49:41.47 +66:34:54.7
06:11:29.09 +72:25:46.6
04:32:07.01 +69:05:36.9
04:07:03.75 +71:00:40.5
03:41:16.99 +68:14:56.9
03:46:59.15 +68:04:12.3
03:58:42.91 +65:14:45.2
03:55:21.86 +67:27:33.4
03:44:35.35 +68:53:12.1
04:00:27.59 +68:34:39.6
04:26:19.36 +74:06:02.6
03:37:03.62 +69:30:34.3
03:49:46.61 +66:14:44.9
03:58:19.27 +68:28:27.8
03:57:23.68 +71:25:00.8
04:27:03.91 +67:43:40.8
04:50:31.21 +70:07:14.5
04:24:09.30 +68:13:54.7
04:23:02.53 +73:36:54.9
04:56:31.45 +72:51:35.0
03:56:53.58 +67:31:31.6
04:16:55.61 +69:09:49.4
04:14:47.37 +68:29:33.3
04:29:19.14 +69:31:54.8
04:45:28.72 +74:16:14.2
04:13:48.14 +71:34:09.6
04:47:41.12 +69:27:48.2
04:32:12.61 +69:46:34.3
03:53:26.02 +65:59:38.2
04:24:11.95 +67:34:11.0
03:51:12.94 +68:31:50.8
06:01:11.09 +71:55:16.4
04:16:55.43 +72:06:22.3
04:24:34.69 +69:53:54.8
04:11:02.10 +73:32:44.3
05:03:03.23 +74:13:01.7
03:53:03.79 +67:44:10.2
04:52:19.78 +69:40:07.4
03:57:21.07 +71:46:52.8
04:01:24.00 +70:57:54.3
05:24:14.97 +70:32:24.4
04:10:46.54 +70:07:35.9
04:24:34.33 +67:41:11.2
03:58:28.05 +72:24:36.8
05:04:54.06 +70:09:41.6
04:12:35.96 +66:58:51.0
04:06:52.94 +65:28:29.8
04:25:21.61 +68:59:43.3
05:03:14.16 +72:34:09.2
04:20:12.28 +67:58:51.8
05:16:13.51 +71:25:49.4
04:56:17.89 +70:32:23.4
04:31:50.03 +66:09:34.8
05:59:26.94 +70:48:57.5
########### Completed Cam-06-Q2b1x1 ###########
The analysis was running at tau
We are allowed to update the exclusion list at tau host
Found ../exclusion_list_TTUQ2.txt
#### The exclusion list before filtering-out asteroids, bad pixels and adding Gaia sources ####
04:49:03.90 +69:07:44.0
06:20:35.20 +72:57:44.3
04:28:03.62 +70:46:00.9
05:15:41.24 +72:19:02.5
04:24:09.95 +70:35:42.9
04:19:02.37 +69:20:47.4
04:20:24.98 +74:02:54.5
04:12:12.07 +72:09:08.5
04:15:21.53 +66:29:41.3
03:50:31.20 +66:54:01.6
04:15:29.39 +66:00:07.2
03:41:01.16 +69:27:18.3
04:01:13.81 +67:58:11.5
04:11:33.42 +65:34:22.7
03:49:41.47 +66:34:54.7
06:11:29.09 +72:25:46.6
04:32:07.01 +69:05:36.9
04:07:03.75 +71:00:40.5
03:41:16.99 +68:14:56.9
03:46:59.15 +68:04:12.3
03:58:42.91 +65:14:45.2
03:55:21.86 +67:27:33.4
03:44:35.35 +68:53:12.1
04:00:27.59 +68:34:39.6
04:26:19.36 +74:06:02.6
03:37:03.62 +69:30:34.3
03:49:46.61 +66:14:44.9
03:58:19.27 +68:28:27.8
03:57:23.68 +71:25:00.8
04:27:03.91 +67:43:40.8
04:50:31.21 +70:07:14.5
04:24:09.30 +68:13:54.7
04:23:02.53 +73:36:54.9
04:56:31.45 +72:51:35.0
03:56:53.58 +67:31:31.6
04:16:55.61 +69:09:49.4
04:14:47.37 +68:29:33.3
04:29:19.14 +69:31:54.8
04:45:28.72 +74:16:14.2
04:13:48.14 +71:34:09.6
04:47:41.12 +69:27:48.2
04:32:12.61 +69:46:34.3
03:53:26.02 +65:59:38.2
04:24:11.95 +67:34:11.0
03:51:12.94 +68:31:50.8
06:01:11.09 +71:55:16.4
04:16:55.43 +72:06:22.3
04:24:34.69 +69:53:54.8
04:11:02.10 +73:32:44.3
05:03:03.23 +74:13:01.7
03:53:03.79 +67:44:10.2
04:52:19.78 +69:40:07.4
03:57:21.07 +71:46:52.8
04:01:24.00 +70:57:54.3
05:24:14.97 +70:32:24.4
04:10:46.54 +70:07:35.9
04:24:34.33 +67:41:11.2
03:58:28.05 +72:24:36.8
05:04:54.06 +70:09:41.6
04:12:35.96 +66:58:51.0
04:06:52.94 +65:28:29.8
04:25:21.61 +68:59:43.3
05:03:14.16 +72:34:09.2
04:20:12.28 +67:58:51.8
05:16:13.51 +71:25:49.4
04:56:17.89 +70:32:23.4
04:31:50.03 +66:09:34.8
05:59:26.94 +70:48:57.5
###################################################################################
04:49:03.90 +69:07:44.0 -- not an asteroid (will add it to exclusion list)
06:20:35.20 +72:57:44.3 -- not an asteroid (will add it to exclusion list)
04:28:03.62 +70:46:00.9 -- not an asteroid (will add it to exclusion list)
05:15:41.24 +72:19:02.5 -- not an asteroid (will add it to exclusion list)
04:24:09.95 +70:35:42.9 -- not an asteroid (will add it to exclusion list)
04:19:02.37 +69:20:47.4 -- not an asteroid (will add it to exclusion list)
04:20:24.98 +74:02:54.5 -- not an asteroid (will add it to exclusion list)
04:12:12.07 +72:09:08.5 -- not an asteroid (will add it to exclusion list)
04:15:21.53 +66:29:41.3 -- not an asteroid (will add it to exclusion list)
03:50:31.20 +66:54:01.6 -- not an asteroid (will add it to exclusion list)
04:15:29.39 +66:00:07.2 -- not an asteroid (will add it to exclusion list)
03:41:01.16 +69:27:18.3 -- not an asteroid (will add it to exclusion list)
04:01:13.81 +67:58:11.5 -- not an asteroid (will add it to exclusion list)
04:11:33.42 +65:34:22.7 -- not an asteroid (will add it to exclusion list)
03:49:41.47 +66:34:54.7 -- not an asteroid (will add it to exclusion list)
06:11:29.09 +72:25:46.6 -- not an asteroid (will add it to exclusion list)
04:32:07.01 +69:05:36.9 -- not an asteroid (will add it to exclusion list)
04:07:03.75 +71:00:40.5 -- not an asteroid (will add it to exclusion list)
03:41:16.99 +68:14:56.9 -- not an asteroid (will add it to exclusion list)
03:46:59.15 +68:04:12.3 -- not an asteroid (will add it to exclusion list)
03:58:42.91 +65:14:45.2 -- not an asteroid (will add it to exclusion list)
03:55:21.86 +67:27:33.4 -- not an asteroid (will add it to exclusion list)
03:44:35.35 +68:53:12.1 -- not an asteroid (will add it to exclusion list)
04:00:27.59 +68:34:39.6 -- not an asteroid (will add it to exclusion list)
04:26:19.36 +74:06:02.6 -- not an asteroid (will add it to exclusion list)
03:37:03.62 +69:30:34.3 -- not an asteroid (will add it to exclusion list)
03:49:46.61 +66:14:44.9 -- not an asteroid (will add it to exclusion list)
03:58:19.27 +68:28:27.8 -- not an asteroid (will add it to exclusion list)
03:57:23.68 +71:25:00.8 -- not an asteroid (will add it to exclusion list)
04:27:03.91 +67:43:40.8 -- not an asteroid (will add it to exclusion list)
04:50:31.21 +70:07:14.5 -- not an asteroid (will add it to exclusion list)
04:24:09.30 +68:13:54.7 -- not an asteroid (will add it to exclusion list)
04:23:02.53 +73:36:54.9 -- not an asteroid (will add it to exclusion list)
04:56:31.45 +72:51:35.0 -- not an asteroid (will add it to exclusion list)
03:56:53.58 +67:31:31.6 -- not an asteroid (will add it to exclusion list)
04:16:55.61 +69:09:49.4 -- not an asteroid (will add it to exclusion list)
04:14:47.37 +68:29:33.3 -- not an asteroid (will add it to exclusion list)
04:29:19.14 +69:31:54.8 -- not an asteroid (will add it to exclusion list)
04:45:28.72 +74:16:14.2 -- not an asteroid (will add it to exclusion list)
04:13:48.14 +71:34:09.6 -- not an asteroid (will add it to exclusion list)
04:47:41.12 +69:27:48.2 -- not an asteroid (will add it to exclusion list)
04:32:12.61 +69:46:34.3 -- not an asteroid (will add it to exclusion list)
03:53:26.02 +65:59:38.2 -- not an asteroid (will add it to exclusion list)
04:24:11.95 +67:34:11.0 -- not an asteroid (will add it to exclusion list)
03:51:12.94 +68:31:50.8 -- not an asteroid (will add it to exclusion list)
06:01:11.09 +71:55:16.4 -- not an asteroid (will add it to exclusion list)
04:16:55.43 +72:06:22.3 -- not an asteroid (will add it to exclusion list)
04:24:34.69 +69:53:54.8 -- not an asteroid (will add it to exclusion list)
04:11:02.10 +73:32:44.3 -- not an asteroid (will add it to exclusion list)
05:03:03.23 +74:13:01.7 -- not an asteroid (will add it to exclusion list)
03:53:03.79 +67:44:10.2 -- not an asteroid (will add it to exclusion list)
04:52:19.78 +69:40:07.4 -- not an asteroid (will add it to exclusion list)
03:57:21.07 +71:46:52.8 -- not an asteroid (will add it to exclusion list)
04:01:24.00 +70:57:54.3 -- not an asteroid (will add it to exclusion list)
05:24:14.97 +70:32:24.4 -- not an asteroid (will add it to exclusion list)
04:10:46.54 +70:07:35.9 -- not an asteroid (will add it to exclusion list)
04:24:34.33 +67:41:11.2 -- not an asteroid (will add it to exclusion list)
03:58:28.05 +72:24:36.8 -- not an asteroid (will add it to exclusion list)
05:04:54.06 +70:09:41.6 -- not an asteroid (will add it to exclusion list)
04:12:35.96 +66:58:51.0 -- not an asteroid (will add it to exclusion list)
04:06:52.94 +65:28:29.8 -- not an asteroid (will add it to exclusion list)
04:25:21.61 +68:59:43.3 -- not an asteroid (will add it to exclusion list)
05:03:14.16 +72:34:09.2 -- not an asteroid (will add it to exclusion list)
04:20:12.28 +67:58:51.8 -- not an asteroid (will add it to exclusion list)
05:16:13.51 +71:25:49.4 -- not an asteroid (will add it to exclusion list)
04:56:17.89 +70:32:23.4 -- not an asteroid (will add it to exclusion list)
04:31:50.03 +66:09:34.8 -- not an asteroid (will add it to exclusion list)
05:59:26.94 +70:48:57.5 -- not an asteroid (will add it to exclusion list)
renamed 'exclusion_list_index_html.txt_noasteroids' -> 'exclusion_list_index_html.txt'
03:37:03.62 +69:30:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:01.16 +69:27:18.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:41:16.99 +68:14:56.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:44:35.35 +68:53:12.1 -- does not seem to be a hot pixel (will add it to exclusion list)
03:46:59.15 +68:04:12.3 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:41.47 +66:34:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
03:49:46.61 +66:14:44.9 -- does not seem to be a hot pixel (will add it to exclusion list)
03:50:31.20 +66:54:01.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:51:12.94 +68:31:50.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:03.79 +67:44:10.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:53:26.02 +65:59:38.2 -- does not seem to be a hot pixel (will add it to exclusion list)
03:55:21.86 +67:27:33.4 -- does not seem to be a hot pixel (will add it to exclusion list)
03:56:53.58 +67:31:31.6 -- does not seem to be a hot pixel (will add it to exclusion list)
03:57:21.07 +71:46:52.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:57:23.68 +71:25:00.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:58:19.27 +68:28:27.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:58:28.05 +72:24:36.8 -- does not seem to be a hot pixel (will add it to exclusion list)
03:58:42.91 +65:14:45.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:00:27.59 +68:34:39.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:01:13.81 +67:58:11.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:01:24.00 +70:57:54.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:06:52.94 +65:28:29.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:07:03.75 +71:00:40.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:10:46.54 +70:07:35.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:11:02.10 +73:32:44.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:11:33.42 +65:34:22.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:12:12.07 +72:09:08.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:12:35.96 +66:58:51.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:13:48.14 +71:34:09.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:14:47.37 +68:29:33.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:15:21.53 +66:29:41.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:15:29.39 +66:00:07.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:16:55.43 +72:06:22.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:16:55.61 +69:09:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:19:02.37 +69:20:47.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:20:12.28 +67:58:51.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:20:24.98 +74:02:54.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:23:02.53 +73:36:54.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:09.30 +68:13:54.7 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:09.95 +70:35:42.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:11.95 +67:34:11.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:34.33 +67:41:11.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:24:34.69 +69:53:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:25:21.61 +68:59:43.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:26:19.36 +74:06:02.6 -- does not seem to be a hot pixel (will add it to exclusion list)
04:27:03.91 +67:43:40.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:28:03.62 +70:46:00.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:29:19.14 +69:31:54.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:31:50.03 +66:09:34.8 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:07.01 +69:05:36.9 -- does not seem to be a hot pixel (will add it to exclusion list)
04:32:12.61 +69:46:34.3 -- does not seem to be a hot pixel (will add it to exclusion list)
04:45:28.72 +74:16:14.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:47:41.12 +69:27:48.2 -- does not seem to be a hot pixel (will add it to exclusion list)
04:49:03.90 +69:07:44.0 -- does not seem to be a hot pixel (will add it to exclusion list)
04:50:31.21 +70:07:14.5 -- does not seem to be a hot pixel (will add it to exclusion list)
04:52:19.78 +69:40:07.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:17.89 +70:32:23.4 -- does not seem to be a hot pixel (will add it to exclusion list)
04:56:31.45 +72:51:35.0 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:03.23 +74:13:01.7 -- does not seem to be a hot pixel (will add it to exclusion list)
05:03:14.16 +72:34:09.2 -- does not seem to be a hot pixel (will add it to exclusion list)
05:04:54.06 +70:09:41.6 -- does not seem to be a hot pixel (will add it to exclusion list)
05:15:41.24 +72:19:02.5 -- does not seem to be a hot pixel (will add it to exclusion list)
05:16:13.51 +71:25:49.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:24:14.97 +70:32:24.4 -- does not seem to be a hot pixel (will add it to exclusion list)
05:59:26.94 +70:48:57.5 -- does not seem to be a hot pixel (will add it to exclusion list)
06:01:11.09 +71:55:16.4 -- does not seem to be a hot pixel (will add it to exclusion list)
06:11:29.09 +72:25:46.6 -- does not seem to be a hot pixel (will add it to exclusion list)
06:20:35.20 +72:57:44.3 -- 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)
03:37:03.62 +69:30:34.3 -- not a known variable star
03:41:01.16 +69:27:18.3 -- not a known variable star
03:41:16.99 +68:14:56.9 -- not a known variable star
03:44:35.35 +68:53:12.1 -- not a known variable star
03:46:59.15 +68:04:12.3 -- not a known variable star
03:49:41.47 +66:34:54.7 -- a known variable star
03:49:46.61 +66:14:44.9 -- not a known variable star
03:50:31.20 +66:54:01.6 -- not a known variable star
03:51:12.94 +68:31:50.8 -- not a known variable star
03:53:03.79 +67:44:10.2 -- a known variable star
03:53:26.02 +65:59:38.2 -- not a known variable star
03:55:21.86 +67:27:33.4 -- not a known variable star
03:56:53.58 +67:31:31.6 -- not a known variable star
03:57:21.07 +71:46:52.8 -- not a known variable star
03:57:23.68 +71:25:00.8 -- not a known variable star
03:58:19.27 +68:28:27.8 -- not a known variable star
03:58:28.05 +72:24:36.8 -- not a known variable star
03:58:42.91 +65:14:45.2 -- not a known variable star
04:00:27.59 +68:34:39.6 -- not a known variable star
04:01:13.81 +67:58:11.5 -- not a known variable star
04:01:24.00 +70:57:54.3 -- not a known variable star
04:06:52.94 +65:28:29.8 -- not a known variable star
04:07:03.75 +71:00:40.5 -- not a known variable star
04:10:46.54 +70:07:35.9 -- not a known variable star
04:11:02.10 +73:32:44.3 -- not a known variable star
04:11:33.42 +65:34:22.7 -- not a known variable star
04:12:12.07 +72:09:08.5 -- not a known variable star
04:12:35.96 +66:58:51.0 -- not a known variable star
04:13:48.14 +71:34:09.6 -- not a known variable star
04:14:47.37 +68:29:33.3 -- not a known variable star
04:15:21.53 +66:29:41.3 -- not a known variable star
04:15:29.39 +66:00:07.2 -- not a known variable star
04:16:55.43 +72:06:22.3 -- not a known variable star
04:16:55.61 +69:09:49.4 -- not a known variable star
04:19:02.37 +69:20:47.4 -- not a known variable star
04:20:12.28 +67:58:51.8 -- not a known variable star
04:20:24.98 +74:02:54.5 -- not a known variable star
04:23:02.53 +73:36:54.9 -- a known variable star
04:24:09.30 +68:13:54.7 -- not a known variable star
04:24:09.95 +70:35:42.9 -- not a known variable star
04:24:11.95 +67:34:11.0 -- not a known variable star
04:24:34.33 +67:41:11.2 -- not a known variable star
04:24:34.69 +69:53:54.8 -- not a known variable star
04:25:21.61 +68:59:43.3 -- a known variable star
04:26:19.36 +74:06:02.6 -- not a known variable star
04:27:03.91 +67:43:40.8 -- not a known variable star
04:28:03.62 +70:46:00.9 -- not a known variable star
04:29:19.14 +69:31:54.8 -- not a known variable star
04:31:50.03 +66:09:34.8 -- not a known variable star
04:32:07.01 +69:05:36.9 -- not a known variable star
04:32:12.61 +69:46:34.3 -- not a known variable star
04:45:28.72 +74:16:14.2 -- not a known variable star
04:47:41.12 +69:27:48.2 -- a known variable star
04:49:03.90 +69:07:44.0 -- not a known variable star
04:50:31.21 +70:07:14.5 -- not a known variable star
04:52:19.78 +69:40:07.4 -- not a known variable star
04:56:17.89 +70:32:23.4 -- not a known variable star
04:56:31.45 +72:51:35.0 -- not a known variable star
05:03:03.23 +74:13:01.7 -- not a known variable star
05:03:14.16 +72:34:09.2 -- not a known variable star
05:04:54.06 +70:09:41.6 -- not a known variable star
05:15:41.24 +72:19:02.5 -- not a known variable star
05:16:13.51 +71:25:49.4 -- not a known variable star
05:24:14.97 +70:32:24.4 -- not a known variable star
05:59:26.94 +70:48:57.5 -- a known variable star
06:01:11.09 +71:55:16.4 -- not a known variable star
06:11:29.09 +72:25:46.6 -- not a known variable star
06:20:35.20 +72:57:44.3 -- not a known variable star
Found 62 unidentified candidates (excluding asteroids, hot pixels and known variable stars).
###################################################################################
68 candidates found (excluding asteroids and hot pixels)
This does not look like a test run
ERROR: too many candidates -- 68 (excluding asteroids and hot pixels), not updating the exclusion list!
###################################################################################
Not allowed to update the exclusion list IS_THIS_TEST_RUN=NO ALLOW_EXCLUSION_LIST_UPDATE= NO
The observatory MPC code is 500
############################################################
Positions of planets computed with util/planet_finder/main.py for JD(UT)2461121.72929418 -observatory 500
22:38:29.68 -07:53:16.6 Mercury (0.9mag)
01:12:10.51 +06:45:56.4 Venus (-3.9mag)
23:06:45.22 -06:51:46.8 Mars (1.2mag)
07:04:56.53 +22:57:47.7 Jupiter (-2.3mag)
00:17:54.71 -00:22:32.4 Saturn (0.9mag)
03:43:07.41 +19:32:30.3 Uranus (5.8mag)
00:07:27.66 -00:36:56.1 Neptune (7.8mag)
20:32:06.86 -22:53:38.0 Pluto (14.5mag)
02:37:54.97 +20:23:36.7 Moon (-9.1mag)
-rw-r--r-- 1 apache apache 361 Mar 22 02:18 planets.txt
############################################################
Positions of selected moons from JPL HORIZONS for JD(UT)2461121.72929418:
07:04:54.11 +22:57:54.8 Io (5.6mag)
07:05:01.70 +22:57:40.5 Europa (5.7mag)
07:04:40.21 +22:58:23.5 Ganymede (5.2mag)
07:04:18.62 +22:58:57.7 Callisto (6.4mag)
07:08:57.51 +22:58:41.4 Himalia (15.2mag)
07:04:52.00 +22:57:55.0 Thebe (16.1mag)
07:08:33.90 +23:22:30.6 Elara (17.2mag)
07:02:09.34 +23:50:49.5 Pasiphae (17.2mag)
07:13:42.97 +22:52:28.4 Carme (18.3mag)
00:17:53.42 -00:22:35.0 Titan (8.8mag)
00:17:58.71 -00:22:22.6 Rhea (10.1mag)
00:18:23.29 -00:20:26.4 Iapetus (11.5mag)
00:18:09.88 -00:22:33.0 Hyperion (14.8mag)
00:19:48.19 -00:11:22.2 Phoebe (16.8mag)
-rw-r--r-- 1 apache apache 569 Mar 22 02:18 moons.txt
############################################################
Positions of selected spacecraft from JPL HORIZONS for JD(UT)2461121.72929418:
13:00:03.16 +07:32:25.8 JWST
18:20:43.78 +29:49:05.3 Chandra
16:56:35.91 -46:19:37.0 XMM-Newton
-rw-r--r-- 1 apache apache 96 Mar 22 02:18 spacecraft.txt
############################################################
Positions of bright comets computed with util/comet_finder/main.py for JD(UT)2461121.72929418 -observatory 500
-rw-r--r-- 1 apache apache 0 Mar 22 02:18 comets.txt
############################################################
List of recent ASAS-SN transients from https://www.astronomy.ohio-state.edu/asassn/transients.html :
13:00:42.99 +37:18:34.60 SN2026fjc 2026-03-19.5 15.97
06:02:44.21 -04:11:06.20 ASASSN-26bv 2026-03-19.19 15.67
12:20:27.90 -45:55:38.40 ASASSN-26bt 2026-03-19.05 16.24
07:49:57.30 -56:14:35.10 ASASSN-26bu 2026-03-19.19 15.74
06:04:29.75 +53:23:34.00 SN 2026eza 2026-03-18.2 17.48
11:54:57.87 +69:19:28.90 AT2026fsf 2026-03-18.14 16.95
10:44:46.95 +58:27:29.30 SN 2026enn 2026-03-18.13 17.53
20:45:54.04 -73:26:43.00 AT 2026ezy 2026-03-18.13 16.83
06:53:18.10 -59:10:49.30 ASASSN-26bs 2026-03-18.02 16.93
07:45:09.29 -62:14:36.20 ASASSN-26br 2026-03-16.16 16.78
19:24:27.93 -52:04:36.40 AT 2023uk 2026-03-16.35 14.2
11:44:44.19 -62:10:45.50 ASASSN-26bq 2026-03-15.03 15.31
04:52:54.50 -15:20:57.10 AT2026fhw 2026-03-14.06 -0.22
11:10:34.24 +02:58:48.10 SN2026drr 2026-03-14.08 0.2
07:26:45.73 -27:45:13.90 ASASSN-26bo 2026-03-14.17 13.8
16:35:46.94 +58:12:28.40 SN2026ebt 2026-03-12.41 17.12
13:01:19.45 +15:42:15.00 SN2026ehe 2026-03-12.11 -0.29
09:15:55.41 +10:08:09.70 SN2026efq 2026-03-12.16 0.06
03:31:20.92 -35:29:29.00 SN2026evh 2026-03-12.05 17.29
06:26:19.15 -85:18:28.10 AT2026ffp 2026-03-12.16 0.37
14:16:42.30 -41:18:36.50 AT2026fij 2026-03-12.05 15.97
10:45:04.71 +00:06:13.10 SN 2026exe 2026-03-11.78 16.48
18:07:45.58 +69:43:01.00 SN2026ess 2026-03-12.37 17.37
13:11:03.58 +49:06:31.80 AT2026ewa 2026-03-12.42 16.77
15:03:25.23 -63:11:22.20 ASASSN-26bp 2026-03-11.92 13.33
13:09:37.25 -35:50:25.20 AT2024cmo 2026-03-11.12 16.29
13:06:01.97 -15:50:14.40 AT2026fdy 2026-03-10.33 16.68
11:30:09.70 -47:26:45.00 ASASSN-26bn 2026-03-10.3 15.14
05:03:25.25 -24:16:50.40 (= Gaia 2026-03-9.09 14.32
03:42:32.53 -04:17:53.70 ASASSN-26bm 2026-03-8.04 15.22
04:31:00.53 -68:29:50.20 ASASSN-26bl 2026-03-7.9 10.26
16:18:17.61 +41:25:11.40 SN 2026dkf 2026-03-6.31 16.7
13:45:00.35 +61:16:50.90 SN 2026ejl 2026-03-6.41 -0.66
09:27:45.48 -37:49:32.80 ASASSN-26bk 2026-03-2.3 13.11
20:22:01.20 +23:47:47.30 ASASSN-26bi 2026-02-28.51 15.86
11:16:22.10 +29:26:22.80 AT2026enm 2026-02-28.39 16.88
08:05:59.83 -48:39:35.60 ASASSN-26bh 2026-02-26.05 14.64
13:24:27.02 -45:57:01.40 ASASSN-26bg 2026-02-26.35 15.28
17:27:50.95 -68:28:46.40 ASASSN-26bf 2026-02-26.3 16.28
18:03:39.29 +19:58:46.30 ASASSN-26be 2026-02-25.56 14.95
17:40:18.19 +07:20:59.60 SN 2026crm 2026-02-24.34 16.9
18:38:36.11 -79:28:58.40 ASASSN-26bb 2026-02-24.36 16.11
17:43:29.75 +11:24:00.60 ASASSN-26bc 2026-02-23.37 -3.37
16:59:41.08 -80:01:51.20 ASASSN-26bd 2026-02-23.3 14.38
11:23:31.77 -08:39:15.40 SN2026cff 2026-02-23.15 -1.08
14:55:17.39 -05:56:05.30 SN2026dmk 2026-02-23.22 -0.76
12:28:15.19 +44:27:20.80 SN2026cjz 2026-02-23.47 15.62
12:12:29.55 -02:40:43.30 AT2026dsk 2026-02-23.4 17.21
09:21:05.29 +06:11:42.80 SN2026chr 2026-02-23.1 17.39
16:05:38.61 +18:06:07.40 SN 2026dsy 2026-02-23.36 17.15
04:55:50.66 -29:52:57.70 SN 2026dpg 2026-02-23.11 15.75
04:21:28.18 -53:22:54.40 AT2026drl 2026-02-21.03 17.31
11:50:37.32 +55:21:13.70 SN 2026dix 2026-02-21.43 16.39
16:21:19.69 -63:47:29.40 ASASSN-26az 2026-02-21.03 17.02
02:45:30.93 -54:17:43.10 SN 2026cju 2026-02-21.04 17.54
01:58:40.68 +47:34:50.10 ASASSN-26av 2026-02-21.09 15.97
18:35:53.01 -42:31:38.90 ASASSN-26aw 2026-02-21.12 15.89
11:40:18.88 -39:45:09.20 ASASSN-26ax 2026-02-21.08 15.73
02:26:23.52 -51:42:29.80 ASASSN-26ay 2026-02-21.04 13.93
08:46:07.66 +01:17:43.90 ASASSN-26ba 2026-02-20.23 15.43
14:15:47.49 -48:05:16.60 SN2026dez 2026-02-19.31 15.91
17:25:53.90 -23:28:31.50 ASASSN-26au 2026-02-18.33 15.82
16:07:59.09 -24:00:10.00 SN2026cmv 2026-02-17.28 16.19
18:15:01.25 -37:43:36.70 ASASSN-26at 2026-02-16.36 15.94
13:01:07.22 -11:25:16.10 AT2026bzh 2026-02-12.16 17.22
10:56:29.81 -07:07:25.30 SN 2026bre 2026-02-12.16 17.15
08:55:43.51 -53:26:11.50 ASASSN-26as 2026-02-12.2 16.54
06:33:50.98 -41:46:25.10 ASASSN-26ar 2026-02-12.04 16.42
12:15:22.43 +23:59:39.60 SN2026bzg 2026-02-11.27 16.32
08:01:10.95 -03:43:14.30 AT2026coj 2026-02-9.25 13.73
12:44:00.18 -57:03:46.80 ASASSN-26aq 2026-02-9.18 16
06:26:33.34 -54:06:39.90 AT2026cih 2026-02-8.06 17.26
23:08:59.40 -88:59:11.60 SN 2026bsu 2026-02-8.03 16.02
01:04:14.94 -62:31:02.30 SN 2026azk 2026-02-8.04 16.41
08:44:55.41 +64:55:09.90 SN 2026anq 2026-02-7.16 17.62
12:37:42.99 +33:26:05.40 SN 2026bnm 2026-02-7.29 16.74
00:12:55.45 +33:21:25.90 SN2026cbh 2026-02-7.09 16.33
08:02:12.64 -04:14:20.90 SN 2026auh 2026-02-7.11 16.64
18:03:52.67 -31:27:26.00 TCP J18035290-3127298 2026-02-7.37 15.76
12:18:03.59 +50:27:10.20 SN 2026bjz 2026-02-7.25 16.48
07:51:51.12 +55:05:27.60 SN 2026ail 2026-02-6.21 16.85
08:10:56.38 +36:49:42.80 AT2026bsa 2026-02-6.29 17.47
04:43:45.47 -15:49:01.00 SN2026azr 2026-02-5.24 16.96
06:14:48.48 -34:20:08.90 ASASSN-26ap 2026-02-5.2 13.77
02:42:33.90 -27:21:02.60 SN 2026aip 2026-02-4.09 15.85
00:43:12.26 +38:35:47.90 AT2026brt 2026-02-3.12 14.92
14:34:27.21 +21:56:59.90 SN2026atb 2026-01-29.32 15.59
13:12:04.11 -60:56:12.40 ASASSN-26ao 2026-01-28.35 15.61
13:00:36.49 -06:28:26.00 SN2026azd 2026-01-28.23 15.69
10:33:50.27 -31:00:53.40 SN 2026ayz 2026-01-25.11 15.3
05:14:22.36 -60:47:20.70 SN 2026apb 2026-01-24.08 17.35
06:39:26.57 -21:49:19.60 AT2026afe 2026-01-23.11 16.17
09:27:23.48 -32:00:31.10 SN 2023kuy 2026-01-21.24 15.33
09:38:44.42 -20:00:54.30 SN2026afi 2026-01-20.24 17.43
06:30:51.41 -74:35:46.80 AT2026ahr 2026-01-20.09 16.98
13:33:03.15 -16:14:28.70 SN2026amc 2026-01-20.29 16.9
06:57:11.13 -17:24:42.80 ASASSN-26an 2026-01-19.31 13.99
17:41:29.59 +68:57:34.90 2026abj 2026-01-18.64 17.02
10:22:25.13 +04:00:01.40 SN 2026kc 2026-01-18.24 16.4
12:42:03.30 +00:41:41.80 SN 2026pg 2026-01-18.5 17.44
-rw-r--r-- 1 apache apache 5.7K Mar 22 02:18 asassn_transients_list.txt
############################################################
Truncated list of TOCP transients from http://www.cbat.eps.harvard.edu/unconf/tocp.html :
15:33:45.28 -22:11:07.3 TCP J15334528-2211073 2026-01-16.8451 14.9mag
22:34:01.26 +39:53:32.8 TCP J22340126+3953328 2026-01-17.5738 16.79Cmag
00:42:52.36 +41:16:13.3 PNV J00425236+4116133 2026-01-18.5502 17.41Cmag
06:57:11.19 -17:24:43.9 TCP J06571119-1724439 2026-01-18.5375 14.2mag
00:42:52.23 +41:01:44.7 PNV J00425223+4101447 2026-01-19.5505 18.74Cmag
09:54:46.47 +69:06:31.7 PNV J09544647+6906317 2026-01-26.8081 19.3mag
18:08:51.99 -26:16:21.9 TCP J18085199-2616219 2026-01-31.8519 12.2mag
08:01:11.02 -03:43:14.1 TCP J08011102-0343141 2026-02-08.8090 15.10Cmag
05:19:15.40 -02:04:51.5 TCP J05191540-0204515 2026-02-13.4306 14.5mag
10:52:41.26 +36:40:08.9 TCP J10524126+3640089 2026-02-17.6065 17.4mag
05:50:50.81 +36:22:45.1 TCP J05505081+3622451 2026-02-17.5511 15.7mag
00:42:51.33 +41:13:49.1 PNV J00425133+4113491 2026-02-20.738 18.3mag
00:43:04.88 +41:29:41.4 PNV J00430488+4129414 2026-02-20.5923 18.84Cmag
17:43:29.74 +11:24:00.3 TCP J17432974+1124003 2026-02-22.3773 13.6mag
09:55:01.59 +69:08:42.7 PNV J09550159+6908427 2026-02-20.893 19.0mag
07:03:25.76 -12:41:40.1 TCP J07032576-1241401 2026-03-10.4268 15.4mag
00:42:36.82 +41:16:05.8 PNV J00423682+4116058 2026-03-12.5744 17.24Cmag
07:26:45.79 -27:45:14.1 TCP J07264579-2745141 2026-03-17.4417 14.8mag
17:57:19.56 -28:08:14.7 TCP J17571956-2808147 2026-03-19.7972 14.5mag
08:46:05.73 +10:47:39.7 TCP J08460573+1047397 2026-03-21.1936 14.5mag
-rw-r--r-- 1 apache apache 187K Mar 22 02:18 tocp_transients_list.txt